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    <title>Recent ucsc_astro_oapolicydeposits items</title>
    <link>https://escholarship.org/uc/ucsc_astro_oapolicydeposits/rss</link>
    <description>Recent eScholarship items from Open Access Policy Deposits</description>
    <pubDate>Sun, 21 Jun 2026 15:59:48 +0000</pubDate>
    <item>
      <title>Climate Action in Higher Education: Roadmap</title>
      <link>https://escholarship.org/uc/item/82f057jt</link>
      <description>The climate crisis and its attendant difficulties present more challenges than any single government, institution or individual can fix. From one perspective, universities and
campus-community members have responded actively, creating new schools and centers, refocusing research, and doing their best to tackle the challenges of a warming world. More practically, however, current efforts are often a siloed mosaic of individual strategies. Time is of the essence – we must face the reality of almost certainly exceeding a 1.5° global temperature rise and potentially a 2.0° rise, if not more. This paper is a call for a more comprehensive, strategic, and coordinated response to the threat of climate change. This white paper presents a bird's-eye view of how a campus’s many components –
administrators, faculty, staff, students, academic departments, interdisciplinary groups, operations units, and outreach services – can work together. Compiling the perspectives of United States and Canadian...</description>
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      <pubDate>Wed, 18 Mar 2026 00:00:00 +0000</pubDate>
      <author>
        <name>Ackerly, David</name>
      </author>
      <author>
        <name>Bales, Roger</name>
      </author>
      <author>
        <name>Blumenthal, George</name>
      </author>
      <author>
        <name>Bunce, Lindsay</name>
      </author>
      <author>
        <name>Bundy, Kevin</name>
      </author>
      <author>
        <name>Criss, Anne</name>
      </author>
      <author>
        <name>Faber, Sandra</name>
      </author>
      <author>
        <name>Forman, Fonna</name>
      </author>
      <author>
        <name>Huising, Mark</name>
      </author>
      <author>
        <name>Lachapelle, Paul</name>
      </author>
      <author>
        <name>Leauthaud, Alexie</name>
      </author>
      <author>
        <name>Leauthaud, Crystele</name>
      </author>
      <author>
        <name>Palkovacs, Eric</name>
      </author>
      <author>
        <name>Pool, Robin</name>
      </author>
      <author>
        <name>Reich, Peter</name>
      </author>
      <author>
        <name>Shaw, Alison</name>
      </author>
      <author>
        <name>Stemen, Mark</name>
      </author>
      <author>
        <name>StClair, Matthew</name>
      </author>
      <author>
        <name>Stoltz, Amanda</name>
      </author>
      <author>
        <name>Zint, Michaela</name>
      </author>
      <author>
        <name>Aron, Adam</name>
      </author>
      <author>
        <name>Arthur, Derede</name>
      </author>
      <author>
        <name>Beck, Michael</name>
      </author>
      <author>
        <name>Burrus, Kai</name>
      </author>
      <author>
        <name>Cavender-Bares, Jeannine</name>
      </author>
      <author>
        <name>Fleischer, Amy</name>
      </author>
      <author>
        <name>Gaensler, Bryan</name>
      </author>
      <author>
        <name>Hseuh, Lily</name>
      </author>
      <author>
        <name>Oberg, Angela</name>
      </author>
      <author>
        <name>Rajagopal, Deepak</name>
      </author>
      <author>
        <name>Sabol, Valerie</name>
      </author>
      <author>
        <name>Samanta, Aritree</name>
      </author>
      <author>
        <name>Shafiei, Fatemeh</name>
      </author>
      <author>
        <name>Stubbs, Christopher</name>
      </author>
    </item>
    <item>
      <title>The Magnificent Five Images of Supernova Refsdal: Time Delay and Magnification Measurements</title>
      <link>https://escholarship.org/uc/item/7281k86f</link>
      <description>In late 2014, four images of supernova (SN) “Refsdal,” the first known example of a strongly lensed SN with multiple resolved images, were detected in the MACS J1149 galaxy-cluster field. Following the images’ discovery, the SN was predicted to reappear within hundreds of days at a new position ∼8″ away in the field. The observed reappearance in late 2015 makes it possible to carry out Refsdal’s original proposal to use a multiply imaged SN to measure the Hubble constant H 0, since the time delay between appearances should vary inversely with H 0. Moreover, the position, brightness, and timing of the reappearance enable a novel test of the blind predictions of galaxy-cluster models, which are typically constrained only by the positions of multiply imaged galaxies. We have developed a new photometry pipeline that uses DOLPHOT to measure the fluxes of the five images of SN Refsdal from difference images. We apply four separate techniques to perform a blind measurement of the relative...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/7281k86f</guid>
      <pubDate>Wed, 11 Mar 2026 00:00:00 +0000</pubDate>
      <author>
        <name>Kelly, Patrick L</name>
      </author>
      <author>
        <name>Rodney, Steven</name>
      </author>
      <author>
        <name>Treu, Tommaso</name>
        <uri>https://orcid.org/0000-0002-8460-0390</uri>
      </author>
      <author>
        <name>Birrer, Simon</name>
      </author>
      <author>
        <name>Bonvin, Vivien</name>
      </author>
      <author>
        <name>Dessart, Luc</name>
      </author>
      <author>
        <name>Foley, Ryan J</name>
        <uri>https://orcid.org/0000-0002-2445-5275</uri>
      </author>
      <author>
        <name>Filippenko, Alexei V</name>
        <uri>https://orcid.org/0000-0003-3460-0103</uri>
      </author>
      <author>
        <name>Gilman, Daniel</name>
      </author>
      <author>
        <name>Jha, Saurabh</name>
      </author>
      <author>
        <name>Hjorth, Jens</name>
      </author>
      <author>
        <name>Mandel, Kaisey</name>
      </author>
      <author>
        <name>Millon, Martin</name>
      </author>
      <author>
        <name>Pierel, Justin</name>
      </author>
      <author>
        <name>Thorp, Stephen</name>
      </author>
      <author>
        <name>Zitrin, Adi</name>
      </author>
      <author>
        <name>Broadhurst, Tom</name>
      </author>
      <author>
        <name>Chen, Wenlei</name>
      </author>
      <author>
        <name>Diego, Jose M</name>
      </author>
      <author>
        <name>Dressler, Alan</name>
      </author>
      <author>
        <name>Graur, Or</name>
      </author>
      <author>
        <name>Jauzac, Mathilde</name>
      </author>
      <author>
        <name>Malkan, Matthew A</name>
        <uri>https://orcid.org/0000-0001-6919-1237</uri>
      </author>
      <author>
        <name>McCully, Curtis</name>
      </author>
      <author>
        <name>Oguri, Masamune</name>
      </author>
      <author>
        <name>Postman, Marc</name>
      </author>
      <author>
        <name>Schmidt, Kasper Borello</name>
      </author>
      <author>
        <name>Sharon, Keren</name>
      </author>
      <author>
        <name>Tucker, Brad E</name>
      </author>
      <author>
        <name>von der Linden, Anja</name>
      </author>
      <author>
        <name>Wambsganss, Joachim</name>
      </author>
    </item>
    <item>
      <title>Cultural violence in news coverage of the George Floyd murder: Exploring media depictions of police brutality toward Black‐Americans</title>
      <link>https://escholarship.org/uc/item/3s81m1zf</link>
      <description>Abstract The 2020 killing of George Floyd by officer Derek Chauvin sparked one of the largest protest movements in the United States. Chauvin was ultimately convicted of murder—a rare but necessary step to police officer accountability for wrongdoing. The media play an important role in framing the public's attitudes surrounding high‐profile cases involving police killings of unarmed civilians. The current study investigates media narratives surrounding the Floyd case for evidence of cultural violence, which occurs when direct, physical violence becomes institutionalized, accepted as normative, and legitimized. We looked for evidence of cultural violence across 300 articles from three U.S. newspapers (i.e., New York Times, Wall Street Journal, and The Star Tribune). We coded for cultural violence themes, which we operationalized as the seven mechanisms of moral disengagement, that is, the process of convincing oneself that ethical standards do not apply. Cultural violence was...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/3s81m1zf</guid>
      <pubDate>Mon, 2 Feb 2026 00:00:00 +0000</pubDate>
      <author>
        <name>Cheek, Jada</name>
      </author>
      <author>
        <name>Bonam, Courtney M</name>
      </author>
      <author>
        <name>Langhout, Regina D</name>
        <uri>https://orcid.org/0000-0001-9607-8539</uri>
      </author>
    </item>
    <item>
      <title>Rethinking Thorne–Żytkow Object Formation: The Fate of X-Ray Binary LMC X-4 and Implications for Ultra-long Gamma-Ray Bursts</title>
      <link>https://escholarship.org/uc/item/982606kw</link>
      <description>We present a start-to-end simulation aimed at studying the long-term fate of high-mass X-ray binaries and whether a Thorne–Żytkow object (TŻO) might ultimately be assembled. We analyze results from a 3D hydrodynamical simulation that models the eventual fate of LMC X-4, a compact high-mass X-ray binary system, after the primary fills its Roche lobe and engulfs the neutron star companion. We discuss the outcome of this engulfment within the standard paradigm of TŻO formation. The post-merger angular momentum content of the stellar core is a key ingredient, as even a small amount of rotation can break spherical symmetry and produce a centrifugally supported accretion disk. Our findings suggest the inspiraling neutron star, upon merging with the core, can accrete efficiently via a disk at high rates (≈10−2 M ⊙ s−1), subsequently collapsing into a black hole and triggering a bright transient with a luminosity and duration typical of an ultra-long gamma-ray burst. We propose that the...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/982606kw</guid>
      <pubDate>Thu, 29 Jan 2026 00:00:00 +0000</pubDate>
      <author>
        <name>Hutchinson-Smith, Tenley</name>
      </author>
      <author>
        <name>Everson, Rosa Wallace</name>
      </author>
      <author>
        <name>Twum, Angela A</name>
      </author>
      <author>
        <name>Batta, Aldo</name>
      </author>
      <author>
        <name>Yarza, Ricardo</name>
        <uri>https://orcid.org/0000-0003-0381-1039</uri>
      </author>
      <author>
        <name>Law-Smith, Jamie AP</name>
      </author>
      <author>
        <name>Vigna-Gómez, Alejandro</name>
      </author>
      <author>
        <name>Ramirez-Ruiz, Enrico</name>
        <uri>https://orcid.org/0000-0003-2558-3102</uri>
      </author>
    </item>
    <item>
      <title>Bremsstrahlung in GRMHD Models of Accreting Black Holes</title>
      <link>https://escholarship.org/uc/item/8831659v</link>
      <description>Bremsstrahlung in GRMHD Models of Accreting Black Holes</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/8831659v</guid>
      <pubDate>Thu, 29 Jan 2026 00:00:00 +0000</pubDate>
      <author>
        <name>Yarza, Ricardo</name>
        <uri>https://orcid.org/0000-0003-0381-1039</uri>
      </author>
      <author>
        <name>Wong, George N</name>
      </author>
      <author>
        <name>Ryan, Benjamin R</name>
      </author>
      <author>
        <name>Gammie, Charles F</name>
      </author>
    </item>
    <item>
      <title>Hydrodynamics and Survivability during Post-main-sequence Planetary Engulfment</title>
      <link>https://escholarship.org/uc/item/8600c286</link>
      <description>The engulfment of substellar bodies (SBs), such as brown dwarfs and planets, by giant stars is a possible explanation for rapidly rotating giants, lithium-rich giants, and the presence of SBs in close orbits around subdwarfs and white dwarfs. We perform three-dimensional hydrodynamical simulations of the flow in the vicinity of an engulfed SB. We model the SB as a rigid body with a reflective surface because it cannot accrete. This reflective boundary changes the flow morphology to resemble that of engulfed compact objects with outflows. We measure the drag coefficients for the ram-pressure and gravitational drag forces acting on the SB, and use them to integrate its trajectory inside the star. We find that engulfment can increase the luminosity of a 1 M ⊙ star by up to a few orders of magnitude. The time for the star to return to its original luminosity is up to a few thousand years when the star has evolved to ≈10 R ⊙ and up to a few decades at the tip of the red giant branch...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/8600c286</guid>
      <pubDate>Thu, 29 Jan 2026 00:00:00 +0000</pubDate>
      <author>
        <name>Yarza, Ricardo</name>
        <uri>https://orcid.org/0000-0003-0381-1039</uri>
      </author>
      <author>
        <name>Razo-López, Naela B</name>
      </author>
      <author>
        <name>Murguia-Berthier, Ariadna</name>
      </author>
      <author>
        <name>Everson, Rosa Wallace</name>
      </author>
      <author>
        <name>Antoni, Andrea</name>
      </author>
      <author>
        <name>MacLeod, Morgan</name>
      </author>
      <author>
        <name>Soares-Furtado, Melinda</name>
      </author>
      <author>
        <name>Lee, Dongwook</name>
      </author>
      <author>
        <name>Ramirez-Ruiz, Enrico</name>
        <uri>https://orcid.org/0000-0003-2558-3102</uri>
      </author>
    </item>
    <item>
      <title>Repeating Partial Tidal Encounters of Sun-like Stars Leading to Their Complete Disruption</title>
      <link>https://escholarship.org/uc/item/6sp9t99f</link>
      <description>Stars grazing supermassive black holes on bound orbits may produce periodic flares over many passages, known as repeating partial tidal disruption events (TDEs). Here, we present 3D hydrodynamic simulations of Sun-like stars over multiple tidal encounters. The star is significantly restructured and becomes less concentrated as a result of mass loss and tidal heating. The vulnerability to mass loss depends sensitively on the stellar density structure, and the strong correlation between the fractional mass loss ΔM/M* and the ratio of the central and average density ρc/ρ¯ , which was initially derived in disruption simulations of main-sequence stars, also applies for stars strongly reshaped by tides. Over multiple orbits, the star loses progressively more mass in each encounter and is doomed to a complete disruption. Throughout its lifetime, the star may produce numerous weak flares (depending on the initial impact parameter), followed by a couple of luminous flares whose brightness...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/6sp9t99f</guid>
      <pubDate>Thu, 29 Jan 2026 00:00:00 +0000</pubDate>
      <author>
        <name>Liu, Chang</name>
      </author>
      <author>
        <name>Yarza, Ricardo</name>
        <uri>https://orcid.org/0000-0003-0381-1039</uri>
      </author>
      <author>
        <name>Ramirez-Ruiz, Enrico</name>
        <uri>https://orcid.org/0000-0003-2558-3102</uri>
      </author>
    </item>
    <item>
      <title>PATOKA: Simulating Electromagnetic Observables of Black Hole Accretion</title>
      <link>https://escholarship.org/uc/item/5pm3z1td</link>
      <description>The Event Horizon Telescope (EHT) has released analyses of reconstructed images of horizon-scale millimeter emission near the supermassive black hole at the center of the M87 galaxy. Parts of the analyses made use of a large library of synthetic black hole images and spectra, which were produced using numerical general relativistic magnetohydrodynamics fluid simulations and polarized ray tracing. In this article, we describe the PATOKA pipeline, which was used to generate the Illinois contribution to the EHT simulation library. We begin by describing the relevant accretion systems and radiative processes. We then describe the details of the three numerical codes we use, iharm, ipole, and igrmonty, paying particular attention to differences between the current generation of the codes and the originally published versions. Finally, we provide a brief overview of simulated data as produced by PATOKA and conclude with a discussion of limitations and future directions.</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/5pm3z1td</guid>
      <pubDate>Thu, 29 Jan 2026 00:00:00 +0000</pubDate>
      <author>
        <name>Wong, George N</name>
      </author>
      <author>
        <name>Prather, Ben S</name>
      </author>
      <author>
        <name>Dhruv, Vedant</name>
      </author>
      <author>
        <name>Ryan, Benjamin R</name>
      </author>
      <author>
        <name>Mościbrodzka, Monika</name>
      </author>
      <author>
        <name>Chan, Chi-kwan</name>
      </author>
      <author>
        <name>Joshi, Abhishek V</name>
      </author>
      <author>
        <name>Yarza, Ricardo</name>
        <uri>https://orcid.org/0000-0003-0381-1039</uri>
      </author>
      <author>
        <name>Ricarte, Angelo</name>
      </author>
      <author>
        <name>Shiokawa, Hotaka</name>
      </author>
      <author>
        <name>Dolence, Joshua C</name>
      </author>
      <author>
        <name>Noble, Scott C</name>
      </author>
      <author>
        <name>McKinney, Jonathan C</name>
      </author>
      <author>
        <name>Gammie, Charles F</name>
      </author>
    </item>
    <item>
      <title>Evolution of the ZTF SLRN-2020 Star-Planet Merger</title>
      <link>https://escholarship.org/uc/item/5fp583w0</link>
      <description>We model the optical and infrared transient ZTF SLRN-2020, previously associated with a star-planet merger. We consider the scenario in which orbital decay via tidal dissipation led to the merger, and we find that tidal heating within the star was likely unobservable in the archival image of the system taken 12 yr before the merger. The observed dust formation months before the merger is consistent with a planet of mass Mp ≳ 5MJ ejecting material as it skims the stellar surface. This interaction gradually intensifies, leading to significant mass ejection on a dynamical timescale (≈hours) as the planet plunges into the stellar interior. Part of the recombination transient associated with this dynamical mass ejection might be inaccessible to the optical observations because its duration (≈hours) is comparable to the cadence. Correspondingly, the observed duration of the transient (≈100 days) is inconsistent with a single episode of dynamical mass ejection. Instead, the transient...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/5fp583w0</guid>
      <pubDate>Thu, 29 Jan 2026 00:00:00 +0000</pubDate>
      <author>
        <name>Yarza, Ricardo</name>
        <uri>https://orcid.org/0000-0003-0381-1039</uri>
      </author>
      <author>
        <name>MacLeod, Morgan</name>
      </author>
      <author>
        <name>Idini, Benjamin</name>
      </author>
      <author>
        <name>Murray-Clay, Ruth</name>
      </author>
      <author>
        <name>Ramirez-Ruiz, Enrico</name>
        <uri>https://orcid.org/0000-0003-2558-3102</uri>
      </author>
    </item>
    <item>
      <title>Chemical Enrichment of Metal-poor Stars Orbiting Massive Black Hole Companions</title>
      <link>https://escholarship.org/uc/item/4h48s3j4</link>
      <description>There are millions of undetected black holes wandering through our galaxy. Observatories like Chandra, LIGO, and more recently, Gaia, have provided valuable insights into the configurations of these elusive objects when residing in binary systems. Motivated by these advances, we study, for the first time, the enhanced accretion of metals from the interstellar medium (ISM) onto low-mass companions in binary systems with highly unequal mass ratios, utilizing a series of hydrodynamical simulations. Our study demonstrates that a stellar companion’s metal accretion history from the ISM alone, from its formation to the present, can significantly influence its surface abundance, especially when enhanced by a massive black hole companion. However, this effect is likely only measurable in stars that are still on the main sequence. Once a stellar companion evolves off the main sequence, similar to what has been observed with the Gaia BH3 companion, the initial dredge-up process is likely...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/4h48s3j4</guid>
      <pubDate>Thu, 29 Jan 2026 00:00:00 +0000</pubDate>
      <author>
        <name>Rosselli-Calderon, Alejandra</name>
      </author>
      <author>
        <name>Stewart, Julia</name>
      </author>
      <author>
        <name>Shen, Sijing</name>
      </author>
      <author>
        <name>Chakrabarti, Sukanya</name>
      </author>
      <author>
        <name>Soares-Furtado, Melinda</name>
      </author>
      <author>
        <name>Ramirez-Ruiz, Enrico</name>
        <uri>https://orcid.org/0000-0003-2558-3102</uri>
      </author>
    </item>
    <item>
      <title>SN 2021foa: The “Flip-flop” Type IIn/Ibn Supernova</title>
      <link>https://escholarship.org/uc/item/4g67k1dr</link>
      <description>We present a comprehensive analysis of the photometric and spectroscopic evolution of SN 2021foa, unique among the class of transitional supernovae for repeatedly changing its spectroscopic appearance from hydrogen-to-helium-to-hydrogen dominated (IIn-to-Ibn-to-IIn) within 50 days past peak brightness. The spectra exhibit multiple narrow (≈300–600 km s−1) absorption lines of hydrogen, helium, calcium, and iron together with broad helium emission lines with a full width at half-maximum (FWHM) of ∼6000 km s−1. For a steady, wind mass-loss regime, light-curve modeling results in an ejecta mass of ∼8 M ⊙ and circumstellar material (CSM) mass below 1 M ⊙, and an ejecta velocity consistent with the FWHM of the broad helium lines. We obtain a mass-loss rate of ≈2 M ⊙ yr−1. This mass-loss rate is 3 orders of magnitude larger than derived for normal Type II supernovae. We estimate that the bulk of the CSM of SN 2021foa must have been expelled within half a year, about 12 yr ago. Our analysis...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/4g67k1dr</guid>
      <pubDate>Thu, 29 Jan 2026 00:00:00 +0000</pubDate>
      <author>
        <name>Farias, D</name>
      </author>
      <author>
        <name>Gall, C</name>
      </author>
      <author>
        <name>Narayan, G</name>
      </author>
      <author>
        <name>Rest, S</name>
      </author>
      <author>
        <name>Villar, VA</name>
      </author>
      <author>
        <name>Angus, CR</name>
      </author>
      <author>
        <name>Auchettl, K</name>
      </author>
      <author>
        <name>Davis, KW</name>
      </author>
      <author>
        <name>Foley, RJ</name>
        <uri>https://orcid.org/0000-0002-2445-5275</uri>
      </author>
      <author>
        <name>Gagliano, A</name>
      </author>
      <author>
        <name>Hjorth, J</name>
      </author>
      <author>
        <name>Izzo, L</name>
      </author>
      <author>
        <name>Kilpatrick, CD</name>
      </author>
      <author>
        <name>Perkins, HML</name>
      </author>
      <author>
        <name>Ramirez-Ruiz, E</name>
        <uri>https://orcid.org/0000-0003-2558-3102</uri>
      </author>
      <author>
        <name>Ransome, CL</name>
      </author>
      <author>
        <name>Sarangi, A</name>
      </author>
      <author>
        <name>Yarza, R</name>
        <uri>https://orcid.org/0000-0003-0381-1039</uri>
      </author>
      <author>
        <name>Coulter, DA</name>
      </author>
      <author>
        <name>Jones, DO</name>
      </author>
      <author>
        <name>Khetan, N</name>
      </author>
      <author>
        <name>Rest, A</name>
      </author>
      <author>
        <name>Siebert, MR</name>
      </author>
      <author>
        <name>Swift, JJ</name>
      </author>
      <author>
        <name>Taggart, K</name>
      </author>
      <author>
        <name>Tinyanont, S</name>
      </author>
      <author>
        <name>Wrubel, P</name>
      </author>
      <author>
        <name>de Boer, TJL</name>
      </author>
      <author>
        <name>Clever, KE</name>
      </author>
      <author>
        <name>Dhara, A</name>
      </author>
      <author>
        <name>Gao, H</name>
      </author>
      <author>
        <name>Lin, C-C</name>
      </author>
    </item>
    <item>
      <title>The Young Supernova Experiment Data Release 1 (YSE DR1): Light Curves and Photometric Classification of 1975 Supernovae</title>
      <link>https://escholarship.org/uc/item/4cv7x8km</link>
      <description>We present the Young Supernova Experiment Data Release 1 (YSE DR1), comprised of processed multicolor PanSTARRS1 griz and Zwicky Transient Facility (ZTF) gr photometry of 1975 transients with host–galaxy associations, redshifts, spectroscopic and/or photometric classifications, and additional data products from 2019 November 24 to 2021 December 20. YSE DR1 spans discoveries and observations from young and fast-rising supernovae (SNe) to transients that persist for over a year, with a redshift distribution reaching z ≈ 0.5. We present relative SN rates from YSE’s magnitude- and volume-limited surveys, which are consistent with previously published values within estimated uncertainties for untargeted surveys. We combine YSE and ZTF data, and create multisurvey SN simulations to train the ParSNIP and SuperRAENN photometric classification algorithms; when validating our ParSNIP classifier on 472 spectroscopically classified YSE DR1 SNe, we achieve 82% accuracy across three SN classes...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/4cv7x8km</guid>
      <pubDate>Thu, 29 Jan 2026 00:00:00 +0000</pubDate>
      <author>
        <name>Aleo, PD</name>
      </author>
      <author>
        <name>Malanchev, K</name>
      </author>
      <author>
        <name>Sharief, S</name>
      </author>
      <author>
        <name>Jones, DO</name>
      </author>
      <author>
        <name>Narayan, G</name>
      </author>
      <author>
        <name>Foley, RJ</name>
        <uri>https://orcid.org/0000-0002-2445-5275</uri>
      </author>
      <author>
        <name>Villar, VA</name>
      </author>
      <author>
        <name>Angus, CR</name>
      </author>
      <author>
        <name>Baldassare, VF</name>
      </author>
      <author>
        <name>Bustamante-Rosell, MJ</name>
      </author>
      <author>
        <name>Chatterjee, D</name>
      </author>
      <author>
        <name>Cold, C</name>
      </author>
      <author>
        <name>Coulter, DA</name>
      </author>
      <author>
        <name>Davis, KW</name>
      </author>
      <author>
        <name>Dhawan, S</name>
      </author>
      <author>
        <name>Drout, MR</name>
      </author>
      <author>
        <name>Engel, A</name>
      </author>
      <author>
        <name>French, KD</name>
      </author>
      <author>
        <name>Gagliano, A</name>
      </author>
      <author>
        <name>Gall, C</name>
      </author>
      <author>
        <name>Hjorth, J</name>
      </author>
      <author>
        <name>Huber, ME</name>
      </author>
      <author>
        <name>Jacobson-Galán, WV</name>
      </author>
      <author>
        <name>Kilpatrick, CD</name>
      </author>
      <author>
        <name>Langeroodi, D</name>
      </author>
      <author>
        <name>Macias, P</name>
        <uri>https://orcid.org/0000-0002-9946-4635</uri>
      </author>
      <author>
        <name>Mandel, KS</name>
      </author>
      <author>
        <name>Margutti, R</name>
        <uri>https://orcid.org/0000-0003-4768-7586</uri>
      </author>
      <author>
        <name>Matasić, F</name>
      </author>
      <author>
        <name>McGill, P</name>
      </author>
      <author>
        <name>Pierel, JDR</name>
      </author>
      <author>
        <name>Ramirez-Ruiz, E</name>
        <uri>https://orcid.org/0000-0003-2558-3102</uri>
      </author>
      <author>
        <name>Ransome, CL</name>
      </author>
      <author>
        <name>Rojas-Bravo, C</name>
      </author>
      <author>
        <name>Siebert, MR</name>
      </author>
      <author>
        <name>Smith, KW</name>
      </author>
      <author>
        <name>de Soto, KM</name>
      </author>
      <author>
        <name>Stroh, MC</name>
      </author>
      <author>
        <name>Tinyanont, S</name>
      </author>
      <author>
        <name>Taggart, K</name>
      </author>
      <author>
        <name>Ward, SM</name>
      </author>
      <author>
        <name>Wojtak, R</name>
      </author>
      <author>
        <name>Auchettl, K</name>
      </author>
      <author>
        <name>Blanchard, PK</name>
      </author>
      <author>
        <name>de Boer, TJL</name>
      </author>
      <author>
        <name>Boyd, BM</name>
      </author>
      <author>
        <name>Carroll, CM</name>
      </author>
      <author>
        <name>Chambers, KC</name>
      </author>
      <author>
        <name>DeMarchi, L</name>
      </author>
      <author>
        <name>Dimitriadis, G</name>
      </author>
      <author>
        <name>Dodd, SA</name>
      </author>
      <author>
        <name>Earl, N</name>
      </author>
      <author>
        <name>Farias, D</name>
      </author>
      <author>
        <name>Gao, H</name>
      </author>
      <author>
        <name>Gomez, S</name>
      </author>
      <author>
        <name>Grayling, M</name>
      </author>
      <author>
        <name>Grillo, C</name>
      </author>
      <author>
        <name>Hayes, EE</name>
      </author>
      <author>
        <name>Hung, T</name>
      </author>
      <author>
        <name>Izzo, L</name>
      </author>
      <author>
        <name>Khetan, N</name>
      </author>
      <author>
        <name>Kolborg, AN</name>
      </author>
      <author>
        <name>Law-Smith, JAP</name>
      </author>
      <author>
        <name>LeBaron, N</name>
      </author>
      <author>
        <name>Lin, C-C</name>
      </author>
      <author>
        <name>Luo, Y</name>
      </author>
      <author>
        <name>Magnier, EA</name>
      </author>
      <author>
        <name>Matthews, D</name>
      </author>
      <author>
        <name>Mockler, B</name>
      </author>
      <author>
        <name>O’Grady, AJG</name>
      </author>
      <author>
        <name>Pan, Y-C</name>
      </author>
      <author>
        <name>Politsch, CA</name>
      </author>
      <author>
        <name>Raimundo, SI</name>
      </author>
      <author>
        <name>Rest, A</name>
      </author>
      <author>
        <name>Ridden-Harper, R</name>
      </author>
      <author>
        <name>Sarangi, A</name>
      </author>
      <author>
        <name>Schrøder, SL</name>
      </author>
      <author>
        <name>Smartt, SJ</name>
      </author>
      <author>
        <name>Terreran, G</name>
      </author>
      <author>
        <name>Thorp, S</name>
      </author>
      <author>
        <name>Vazquez, J</name>
      </author>
      <author>
        <name>Wainscoat, RJ</name>
      </author>
      <author>
        <name>Wang, Q</name>
      </author>
      <author>
        <name>Wasserman, AR</name>
      </author>
      <author>
        <name>Yadavalli, SK</name>
      </author>
      <author>
        <name>Yarza, R</name>
        <uri>https://orcid.org/0000-0003-0381-1039</uri>
      </author>
      <author>
        <name>Zenati, Y</name>
      </author>
    </item>
    <item>
      <title>The Evolution of Binaries Embedded Within Common Envelopes</title>
      <link>https://escholarship.org/uc/item/3zv8t7gk</link>
      <description>Triple stellar systems allow us to study stellar processes that cannot be attained in binary stars. The evolutionary phases in which the stellar members undergo mass exchanges can alter the hierarchical layout of these systems. Yet, the lack of a self-consistent treatment of common-envelope (CE) in triple-star systems hinders the comprehensive understanding of their long-term fate. This paper examines the conditions predicted around binaries embedded within CEs using local 3D hydrodynamical simulations. We explore varying the initial binary separation, the flow Mach number, and the background stellar density gradients as informed by a wide array of CE conditions, including those invoked to explain the formation of the triple system hosting PSR J0337+1715. We find that the stellar density gradient governs the gaseous drag force, which determines the final configuration of the embedded binary. We observe a comparable net drag force on the center of mass but an overall reduction...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/3zv8t7gk</guid>
      <pubDate>Thu, 29 Jan 2026 00:00:00 +0000</pubDate>
      <author>
        <name>Rosselli-Calderon, Alejandra</name>
      </author>
      <author>
        <name>Yarza, Ricardo</name>
        <uri>https://orcid.org/0000-0003-0381-1039</uri>
      </author>
      <author>
        <name>Murguia-Berthier, Ariadna</name>
      </author>
      <author>
        <name>Rohoza, Valeriia</name>
      </author>
      <author>
        <name>Everson, Rosa Wallace</name>
      </author>
      <author>
        <name>Antoni, Andrea</name>
      </author>
      <author>
        <name>MacLeod, Morgan</name>
      </author>
      <author>
        <name>Ramirez-Ruiz, Enrico</name>
        <uri>https://orcid.org/0000-0003-2558-3102</uri>
      </author>
    </item>
    <item>
      <title>&lt;i&gt;K2&lt;/i&gt; Study of the Magnetic Precataclysmic Variable V1082 Sagittarius</title>
      <link>https://escholarship.org/uc/item/3v32g9hg</link>
      <description>&lt;i&gt;K2&lt;/i&gt; Study of the Magnetic Precataclysmic Variable V1082 Sagittarius</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/3v32g9hg</guid>
      <pubDate>Thu, 29 Jan 2026 00:00:00 +0000</pubDate>
      <author>
        <name>Tovmassian, Gagik</name>
      </author>
      <author>
        <name>Szkody, Paula</name>
      </author>
      <author>
        <name>Yarza, Ricardo</name>
        <uri>https://orcid.org/0000-0003-0381-1039</uri>
      </author>
      <author>
        <name>Kennedy, Mark</name>
      </author>
    </item>
    <item>
      <title>SN 2023ixf in Messier 101: The Twilight Years of the Progenitor as Seen by Pan-STARRS</title>
      <link>https://escholarship.org/uc/item/3hm9q827</link>
      <description>The nearby type II supernova, SN 2023ixf in M101 exhibits signatures of early time interaction with circumstellar material in the first week postexplosion. This material may be the consequence of prior mass loss suffered by the progenitor, which possibly manifested in the form of a detectable presupernova outburst. We present an analysis of long-baseline preexplosion photometric data in the g, w, r, i, z, and y filters from Pan-STARRS as part of the Young Supernova Experiment, spanning ∼5000 days. We find no significant detections in the Pan-STARRS preexplosion light curves. We train a multilayer perceptron neural network to classify presupernova outbursts. We find no evidence of eruptive presupernova activity to a limiting absolute magnitude of −7 mag. The limiting magnitudes from the full set of gwrizy (average absolute magnitude ≈ −8 mag) data are consistent with previous preexplosion studies. We use deep photometry from the literature to constrain the progenitor of SN 2023ixf,...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/3hm9q827</guid>
      <pubDate>Thu, 29 Jan 2026 00:00:00 +0000</pubDate>
      <author>
        <name>Ransome, Conor L</name>
      </author>
      <author>
        <name>Villar, V Ashley</name>
      </author>
      <author>
        <name>Tartaglia, Anna</name>
      </author>
      <author>
        <name>Gonzalez, Sebastian Javier</name>
      </author>
      <author>
        <name>Jacobson-Galán, Wynn V</name>
      </author>
      <author>
        <name>Kilpatrick, Charles D</name>
      </author>
      <author>
        <name>Margutti, Raffaella</name>
        <uri>https://orcid.org/0000-0003-4768-7586</uri>
      </author>
      <author>
        <name>Foley, Ryan J</name>
        <uri>https://orcid.org/0000-0002-2445-5275</uri>
      </author>
      <author>
        <name>Grayling, Matthew</name>
      </author>
      <author>
        <name>Ni, Yuan Qi</name>
      </author>
      <author>
        <name>Yarza, Ricardo</name>
        <uri>https://orcid.org/0000-0003-0381-1039</uri>
      </author>
      <author>
        <name>Ye, Christine</name>
      </author>
      <author>
        <name>Auchettl, Katie</name>
      </author>
      <author>
        <name>de Boer, Thomas</name>
      </author>
      <author>
        <name>Chambers, Kenneth C</name>
      </author>
      <author>
        <name>Coulter, David A</name>
      </author>
      <author>
        <name>Drout, Maria R</name>
      </author>
      <author>
        <name>Farias, Diego</name>
      </author>
      <author>
        <name>Gall, Christa</name>
      </author>
      <author>
        <name>Gao, Hua</name>
      </author>
      <author>
        <name>Huber, Mark E</name>
      </author>
      <author>
        <name>Ibik, Adaeze L</name>
      </author>
      <author>
        <name>Jones, David O</name>
      </author>
      <author>
        <name>Khetan, Nandita</name>
      </author>
      <author>
        <name>Lin, Chien-Cheng</name>
      </author>
      <author>
        <name>Politsch, Collin A</name>
      </author>
      <author>
        <name>Raimundo, Sandra I</name>
      </author>
      <author>
        <name>Rest, Armin</name>
      </author>
      <author>
        <name>Wainscoat, Richard J</name>
      </author>
      <author>
        <name>Yadavalli, S Karthik</name>
      </author>
      <author>
        <name>Zenati, Yossef</name>
      </author>
    </item>
    <item>
      <title>Tidal Disruption Events from Eccentric Orbits and Lessons Learned from the Noteworthy ASASSN-14ko</title>
      <link>https://escholarship.org/uc/item/3fr474b4</link>
      <description>Stars grazing supermassive black holes (SMBHs) on bound orbits may survive tidal disruption, causing periodic flares. Inspired by the recent discovery of the periodic nuclear transient ASASSN-14ko, a promising candidate for a repeating tidal disruption event (TDE), we study the tidal deformation of stars approaching SMBHs on eccentric orbits. With both analytical and hydrodynamic methods, we show the overall tidal deformation of a star is similar to that in a parabolic orbit provided that the eccentricity is above a critical value. This allows one to make use of existing simulation libraries from parabolic encounters to calculate the mass fallback rate in eccentric TDEs. We find the flare structures of eccentric TDEs show a complicated dependence on both the SMBH mass and the orbital period. For stars orbiting SMBHs with relatively short periods, we predict significantly shorter-lived duration flares than those in parabolic TDEs, which can be used to predict repeating events if...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/3fr474b4</guid>
      <pubDate>Thu, 29 Jan 2026 00:00:00 +0000</pubDate>
      <author>
        <name>Liu, Chang</name>
      </author>
      <author>
        <name>Mockler, Brenna</name>
      </author>
      <author>
        <name>Ramirez-Ruiz, Enrico</name>
        <uri>https://orcid.org/0000-0003-2558-3102</uri>
      </author>
      <author>
        <name>Yarza, Ricardo</name>
        <uri>https://orcid.org/0000-0003-0381-1039</uri>
      </author>
      <author>
        <name>Law-Smith, Jamie AP</name>
      </author>
      <author>
        <name>Naoz, Smadar</name>
      </author>
      <author>
        <name>Melchor, Denyz</name>
      </author>
      <author>
        <name>Rose, Sanaea</name>
      </author>
    </item>
    <item>
      <title>TESS Hunt for Young and Maturing Exoplanets (THYME). XI. An Earth-sized Planet Orbiting a Nearby, Solar-like Host in the 400 Myr Ursa Major Moving Group</title>
      <link>https://escholarship.org/uc/item/28m2j3d2</link>
      <description>Young terrestrial worlds are critical test beds to constrain prevailing theories of planetary formation and evolution. We present the discovery of HD 63433 d—a nearby (22 pc), Earth-sized planet transiting a young Sun-like star (TOI-1726, HD 63433). HD 63433 d is the third planet detected in this multiplanet system. The kinematic, rotational, and abundance properties of the host star indicate that it belongs to the young (414 ± 23 Myr) Ursa Major moving group, whose membership we update using new data from the third data release of the Gaia mission and TESS. Our transit analysis of the TESS light curves indicates that HD 63433 d has a radius of 1.1 R ⊕ and closely orbits its host star with a period of 4.2 days. To date, HD 63433 d is the smallest confirmed exoplanet with an age less than 500 Myr, and the nearest young Earth-sized planet. Furthermore, the apparent brightness of the stellar host (V ≃ 6.9 mag) makes this transiting multiplanet system favorable to further investigations,...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/28m2j3d2</guid>
      <pubDate>Thu, 29 Jan 2026 00:00:00 +0000</pubDate>
      <author>
        <name>Capistrant, Benjamin K</name>
      </author>
      <author>
        <name>Soares-Furtado, Melinda</name>
      </author>
      <author>
        <name>Vanderburg, Andrew</name>
      </author>
      <author>
        <name>Jankowski, Alyssa</name>
      </author>
      <author>
        <name>Mann, Andrew W</name>
      </author>
      <author>
        <name>Ross, Gabrielle</name>
      </author>
      <author>
        <name>Srdoc, Gregor</name>
      </author>
      <author>
        <name>Hinkel, Natalie R</name>
      </author>
      <author>
        <name>Becker, Juliette</name>
      </author>
      <author>
        <name>Magliano, Christian</name>
      </author>
      <author>
        <name>Limbach, Mary Anne</name>
      </author>
      <author>
        <name>Stephan, Alexander P</name>
      </author>
      <author>
        <name>Nine, Andrew C</name>
      </author>
      <author>
        <name>Tofflemire, Benjamin M</name>
      </author>
      <author>
        <name>Kraus, Adam L</name>
      </author>
      <author>
        <name>Giacalone, Steven</name>
      </author>
      <author>
        <name>Winn, Joshua N</name>
      </author>
      <author>
        <name>Bieryla, Allyson</name>
      </author>
      <author>
        <name>Bouma, Luke G</name>
      </author>
      <author>
        <name>Ciardi, David R</name>
      </author>
      <author>
        <name>Collins, Karen A</name>
      </author>
      <author>
        <name>Covone, Giovanni</name>
      </author>
      <author>
        <name>de Beurs, Zoë L</name>
      </author>
      <author>
        <name>Huang, Chelsea X</name>
      </author>
      <author>
        <name>Jenkins, Jon M</name>
      </author>
      <author>
        <name>Kreidberg, Laura</name>
      </author>
      <author>
        <name>Latham, David W</name>
      </author>
      <author>
        <name>Quinn, Samuel N</name>
      </author>
      <author>
        <name>Seager, Sara</name>
      </author>
      <author>
        <name>Shporer, Avi</name>
      </author>
      <author>
        <name>Twicken, Joseph D</name>
      </author>
      <author>
        <name>Wohler, Bill</name>
      </author>
      <author>
        <name>Vanderspek, Roland K</name>
      </author>
      <author>
        <name>Yarza, Ricardo</name>
        <uri>https://orcid.org/0000-0003-0381-1039</uri>
      </author>
      <author>
        <name>Ziegler, Carl</name>
      </author>
    </item>
    <item>
      <title>Black Hole Survival Guide: Searching for Stars in the Galactic Center that Endure Partial Tidal Disruption</title>
      <link>https://escholarship.org/uc/item/0mc3f3x0</link>
      <description>Once per ≈104–105 yr, an unlucky star may experience a close encounter with a supermassive black hole (SMBH), partially or fully tearing apart the star in an exceedingly brief, bright interaction called a tidal disruption event (TDE). Remnants of partial TDEs are expected to be plentiful in our Galactic center, where at least six unexplained, diffuse, star-like “G objects” have already been detected, which may have formed via interactions between stars and the SMBH. Using numerical simulations, this work aims to identify the characteristics of TDE remnants. We take 3D hydrodynamic FLASH models of partially disrupted stars and map them into the 1D stellar evolution code MESA to examine the properties of these remnants from tens to billions of years after the TDE. The remnants initially exhibit a brief, highly luminous phase, followed by an extended cooling period as they return to stable hydrogen burning. During the initial stage (≲105 yr) their luminosities increase by orders...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/0mc3f3x0</guid>
      <pubDate>Thu, 29 Jan 2026 00:00:00 +0000</pubDate>
      <author>
        <name>Bush, Rewa Clark</name>
      </author>
      <author>
        <name>Wu, Samantha C</name>
      </author>
      <author>
        <name>Everson, Rosa Wallace</name>
      </author>
      <author>
        <name>Yarza, Ricardo</name>
        <uri>https://orcid.org/0000-0003-0381-1039</uri>
      </author>
      <author>
        <name>Murguia-Berthier, Ariadna</name>
      </author>
      <author>
        <name>Ramirez-Ruiz, Enrico</name>
        <uri>https://orcid.org/0000-0003-2558-3102</uri>
      </author>
    </item>
    <item>
      <title>The Draco Dwarf Spheroidal Galaxy in the First Year of Dark Energy Spectroscopic Instrument Data</title>
      <link>https://escholarship.org/uc/item/5616n854</link>
      <description>We investigate the spatial distribution, kinematics, and metallicity of stars in the Draco dwarf spheroidal galaxy using data from the Dark Energy Spectroscopic Instrument (DESI). We identify 155 high-probability members of Draco using line-of-sight velocity and metallicity information derived from DESI spectroscopy along with Gaia Data Release 3 proper motions. We find a mean line-of-sight velocity of −290.62 ± 0.80 km s−1 with dispersion = 9.57−0.62+0.66 km s−1 and mean metallicity [Fe/H] = −2.10 ± 0.04, consistent with previous results. We also find that Draco has a steep metallicity gradient within the half-light radius, and a metallicity gradient that flattens beyond the half-light radius. We identify eight high-probability members outside the King tidal radius, four of which we identify for the first time. These extratidal stars are not preferentially aligned along the orbit of Draco. We compute an average surface brightness of 34.02 mag arcsec−2 within an elliptical annulus...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/5616n854</guid>
      <pubDate>Wed, 17 Dec 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Ding, J</name>
      </author>
      <author>
        <name>Rockosi, C</name>
      </author>
      <author>
        <name>Li, Ting S</name>
      </author>
      <author>
        <name>Koposov, SE</name>
      </author>
      <author>
        <name>Riley, AH</name>
      </author>
      <author>
        <name>Wang, W</name>
      </author>
      <author>
        <name>Cooper, AP</name>
      </author>
      <author>
        <name>Kizhuprakkat, N</name>
      </author>
      <author>
        <name>Lambert, M</name>
        <uri>https://orcid.org/0000-0002-2527-8899</uri>
      </author>
      <author>
        <name>Medina, GE</name>
      </author>
      <author>
        <name>Sandford, N</name>
      </author>
      <author>
        <name>Aguilar, J</name>
      </author>
      <author>
        <name>Ahlen, S</name>
      </author>
      <author>
        <name>Bianchi, D</name>
      </author>
      <author>
        <name>Brooks, D</name>
      </author>
      <author>
        <name>Claybaugh, T</name>
      </author>
      <author>
        <name>de la Macorra, A</name>
      </author>
      <author>
        <name>Doel, P</name>
      </author>
      <author>
        <name>Forero-Romero, JE</name>
      </author>
      <author>
        <name>Gaztañaga, E</name>
      </author>
      <author>
        <name>Gontcho, S Gontcho A</name>
      </author>
      <author>
        <name>Gutierrez, G</name>
      </author>
      <author>
        <name>Guy, J</name>
        <uri>https://orcid.org/0000-0001-9822-6793</uri>
      </author>
      <author>
        <name>Ishak, M</name>
      </author>
      <author>
        <name>Kehoe, R</name>
      </author>
      <author>
        <name>Kisner, T</name>
      </author>
      <author>
        <name>Kremin, A</name>
        <uri>https://orcid.org/0000-0003-0667-5941</uri>
      </author>
      <author>
        <name>Lahav, O</name>
      </author>
      <author>
        <name>Landriau, M</name>
        <uri>https://orcid.org/0000-0003-1838-8528</uri>
      </author>
      <author>
        <name>Le Guillou, L</name>
      </author>
      <author>
        <name>Meisner, A</name>
      </author>
      <author>
        <name>Miquel, R</name>
      </author>
      <author>
        <name>Moustakas, J</name>
      </author>
      <author>
        <name>Prada, F</name>
      </author>
      <author>
        <name>Pérez-Ràfols, I</name>
      </author>
      <author>
        <name>Rossi, G</name>
      </author>
      <author>
        <name>Sanchez, E</name>
      </author>
      <author>
        <name>Schubnell, M</name>
      </author>
      <author>
        <name>Silber, J</name>
        <uri>https://orcid.org/0000-0002-3461-0320</uri>
      </author>
      <author>
        <name>Sprayberry, D</name>
      </author>
      <author>
        <name>Tarlé, G</name>
      </author>
      <author>
        <name>Weaver, BA</name>
      </author>
      <author>
        <name>Zhou, R</name>
        <uri>https://orcid.org/0000-0001-5381-4372</uri>
      </author>
    </item>
    <item>
      <title>The Hourglass Simulation: A Catalog for the Roman High-latitude Time-domain Core Community Survey</title>
      <link>https://escholarship.org/uc/item/2p84t4bs</link>
      <description>We present a simulation of the time-domain catalog for the Nancy Grace Roman Space Telescope’s High-Latitude Time-Domain Core Community Survey. This simulation, called the Hourglass simulation, uses the most up-to-date spectral energy distribution models and rate measurements for 10 extragalactic time-domain sources. We simulate these models through the design reference Roman Space Telescope survey: four filters per tier, a five-day cadence, over 2 yr, a wide tier of 19 deg&lt;sup&gt;2&lt;/sup&gt;, and a deep tier of 4.2 deg&lt;sup&gt;2&lt;/sup&gt;, with ∼20% of those areas also covered with prism observations. We find that a science-independent Roman time-domain catalog, assuming a signal-to-noise ratio at a max of &amp;gt;5, would have approximately 21,000 Type Ia supernovae, 40,000 core-collapse supernovae, around 70 superluminous supernovae, ∼35 tidal disruption events, three kilonovae, and possibly pair-instability supernovae. In total, Hourglass has over 64,000 transient objects, 11,000,000 photometric...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/2p84t4bs</guid>
      <pubDate>Wed, 24 Sep 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Rose, BM</name>
      </author>
      <author>
        <name>Vincenzi, M</name>
      </author>
      <author>
        <name>Hounsell, R</name>
      </author>
      <author>
        <name>Qu, H</name>
      </author>
      <author>
        <name>Aldoroty, L</name>
      </author>
      <author>
        <name>Scolnic, D</name>
      </author>
      <author>
        <name>Kessler, R</name>
      </author>
      <author>
        <name>Macias, P</name>
        <uri>https://orcid.org/0000-0002-9946-4635</uri>
      </author>
      <author>
        <name>Brout, D</name>
      </author>
      <author>
        <name>Acevedo, M</name>
      </author>
      <author>
        <name>Chen, RC</name>
      </author>
      <author>
        <name>Gomez, S</name>
      </author>
      <author>
        <name>Peterson, E</name>
      </author>
      <author>
        <name>Rubin, D</name>
      </author>
      <author>
        <name>Sako, M</name>
      </author>
      <author>
        <name>Team, the Roman Supernova Project Infrastructure</name>
      </author>
    </item>
    <item>
      <title>Cosmological Results from the RAISIN Survey: Using Type Ia Supernovae in the Near Infrared as a Novel Path to Measure the Dark Energy Equation of State</title>
      <link>https://escholarship.org/uc/item/6s5221nh</link>
      <description>Type Ia supernovae (SNe Ia) are more precise standardizable candles when measured in the near-infrared (NIR) than in the optical. With this motivation, from 2012 to 2017 we embarked on the RAISIN program with the Hubble Space Telescope (HST) to obtain rest-frame NIR light curves for a cosmologically distant sample of 37 SNe Ia (0.2 ≤ z ≤ 0.6) discovered by Pan-STARRS and the Dark Energy Survey. By comparing higher-z HST data with 42 SNe Ia at z &amp;lt; 0.1 observed in the NIR by the Carnegie Supernova Project, we construct a Hubble diagram from NIR observations (with only time of maximum light and some selection cuts from optical photometry) to pursue a unique avenue to constrain the dark energy equation-of-state parameter, w. We analyze the dependence of the full set of Hubble residuals on the SN Ia host galaxy mass and find Hubble residual steps of size ∼0.06-0.1 mag with 1.5σ-2.5σ significance depending on the method and step location used. Combining our NIR sample with cosmic...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/6s5221nh</guid>
      <pubDate>Mon, 22 Sep 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Jones, DO</name>
      </author>
      <author>
        <name>Mandel, KS</name>
      </author>
      <author>
        <name>Kirshner, RP</name>
      </author>
      <author>
        <name>Thorp, S</name>
      </author>
      <author>
        <name>Challis, PM</name>
      </author>
      <author>
        <name>Avelino, A</name>
      </author>
      <author>
        <name>Brout, D</name>
      </author>
      <author>
        <name>Burns, C</name>
      </author>
      <author>
        <name>Foley, RJ</name>
        <uri>https://orcid.org/0000-0002-2445-5275</uri>
      </author>
      <author>
        <name>Pan, Y-C</name>
      </author>
      <author>
        <name>Scolnic, DM</name>
      </author>
      <author>
        <name>Siebert, MR</name>
      </author>
      <author>
        <name>Chornock, R</name>
        <uri>https://orcid.org/0000-0002-7706-5668</uri>
      </author>
      <author>
        <name>Freedman, WL</name>
      </author>
      <author>
        <name>Friedman, A</name>
      </author>
      <author>
        <name>Frieman, J</name>
      </author>
      <author>
        <name>Galbany, L</name>
      </author>
      <author>
        <name>Hsiao, E</name>
      </author>
      <author>
        <name>Kelsey, L</name>
      </author>
      <author>
        <name>Marion, GH</name>
      </author>
      <author>
        <name>Nichol, RC</name>
      </author>
      <author>
        <name>Nugent, PE</name>
        <uri>https://orcid.org/0000-0002-3389-0586</uri>
      </author>
      <author>
        <name>Phillips, MM</name>
      </author>
      <author>
        <name>Rest, A</name>
      </author>
      <author>
        <name>Riess, AG</name>
      </author>
      <author>
        <name>Sako, M</name>
      </author>
      <author>
        <name>Smith, M</name>
      </author>
      <author>
        <name>Wiseman, P</name>
      </author>
      <author>
        <name>Wood-Vasey, WM</name>
      </author>
    </item>
    <item>
      <title>The Dark Energy Survey: Cosmology Results with ∼1500 New High-redshift Type Ia Supernovae Using the Full 5 yr Data Set</title>
      <link>https://escholarship.org/uc/item/498713kh</link>
      <description>We present cosmological constraints from the sample of Type Ia supernovae (SNe Ia) discovered and measured during the full 5 yr of the Dark Energy Survey (DES) SN program. In contrast to most previous cosmological samples, in which SNe are classified based on their spectra, we classify the DES SNe using a machine learning algorithm applied to their light curves in four photometric bands. Spectroscopic redshifts are acquired from a dedicated follow-up survey of the host galaxies. After accounting for the likelihood of each SN being an SN Ia, we find 1635 DES SNe in the redshift range 0.10 &amp;lt; z &amp;lt; 1.13 that pass quality selection criteria sufficient to constrain cosmological parameters. This quintuples the number of high-quality z &amp;gt; 0.5 SNe compared to the previous leading compilation of Pantheon+ and results in the tightest cosmological constraints achieved by any SN data set to date. To derive cosmological constraints, we combine the DES SN data with a high-quality external...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/498713kh</guid>
      <pubDate>Wed, 30 Jul 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Abbott, DES Collaboration TMC</name>
      </author>
      <author>
        <name>Acevedo, M</name>
      </author>
      <author>
        <name>Aguena, M</name>
      </author>
      <author>
        <name>Alarcon, A</name>
      </author>
      <author>
        <name>Allam, S</name>
      </author>
      <author>
        <name>Alves, O</name>
      </author>
      <author>
        <name>Amon, A</name>
      </author>
      <author>
        <name>Andrade-Oliveira, F</name>
      </author>
      <author>
        <name>Annis, J</name>
      </author>
      <author>
        <name>Armstrong, P</name>
      </author>
      <author>
        <name>Asorey, J</name>
      </author>
      <author>
        <name>Avila, S</name>
      </author>
      <author>
        <name>Bacon, D</name>
      </author>
      <author>
        <name>Bassett, BA</name>
      </author>
      <author>
        <name>Bechtol, K</name>
      </author>
      <author>
        <name>Bernardinelli, PH</name>
      </author>
      <author>
        <name>Bernstein, GM</name>
      </author>
      <author>
        <name>Bertin, E</name>
      </author>
      <author>
        <name>Blazek, J</name>
      </author>
      <author>
        <name>Bocquet, S</name>
      </author>
      <author>
        <name>Brooks, D</name>
      </author>
      <author>
        <name>Brout, D</name>
      </author>
      <author>
        <name>Buckley-Geer, E</name>
      </author>
      <author>
        <name>Burke, DL</name>
      </author>
      <author>
        <name>Camacho, H</name>
      </author>
      <author>
        <name>Camilleri, R</name>
      </author>
      <author>
        <name>Campos, A</name>
      </author>
      <author>
        <name>Rosell, A Carnero</name>
      </author>
      <author>
        <name>Carollo, D</name>
      </author>
      <author>
        <name>Carr, A</name>
      </author>
      <author>
        <name>Carretero, J</name>
      </author>
      <author>
        <name>Castander, FJ</name>
      </author>
      <author>
        <name>Cawthon, R</name>
      </author>
      <author>
        <name>Chang, C</name>
      </author>
      <author>
        <name>Chen, R</name>
      </author>
      <author>
        <name>Choi, A</name>
      </author>
      <author>
        <name>Conselice, C</name>
      </author>
      <author>
        <name>Costanzi, M</name>
      </author>
      <author>
        <name>da Costa, LN</name>
      </author>
      <author>
        <name>Crocce, M</name>
      </author>
      <author>
        <name>Davis, TM</name>
      </author>
      <author>
        <name>DePoy, DL</name>
      </author>
      <author>
        <name>Desai, S</name>
      </author>
      <author>
        <name>Diehl, HT</name>
      </author>
      <author>
        <name>Dixon, M</name>
      </author>
      <author>
        <name>Dodelson, S</name>
      </author>
      <author>
        <name>Doel, P</name>
      </author>
      <author>
        <name>Doux, C</name>
      </author>
      <author>
        <name>Drlica-Wagner, A</name>
      </author>
      <author>
        <name>Elvin-Poole, J</name>
      </author>
      <author>
        <name>Everett, S</name>
      </author>
      <author>
        <name>Ferrero, I</name>
      </author>
      <author>
        <name>Ferté, A</name>
      </author>
      <author>
        <name>Flaugher, B</name>
      </author>
      <author>
        <name>Foley, RJ</name>
        <uri>https://orcid.org/0000-0002-2445-5275</uri>
      </author>
      <author>
        <name>Fosalba, P</name>
      </author>
      <author>
        <name>Friedel, D</name>
      </author>
      <author>
        <name>Frieman, J</name>
      </author>
      <author>
        <name>Frohmaier, C</name>
      </author>
      <author>
        <name>Galbany, L</name>
      </author>
      <author>
        <name>García-Bellido, J</name>
      </author>
      <author>
        <name>Gatti, M</name>
      </author>
      <author>
        <name>Gaztanaga, E</name>
      </author>
      <author>
        <name>Giannini, G</name>
      </author>
      <author>
        <name>Glazebrook, K</name>
      </author>
      <author>
        <name>Graur, O</name>
      </author>
      <author>
        <name>Gruen, D</name>
      </author>
      <author>
        <name>Gruendl, RA</name>
      </author>
      <author>
        <name>Gutierrez, G</name>
      </author>
      <author>
        <name>Hartley, WG</name>
      </author>
      <author>
        <name>Herner, K</name>
      </author>
      <author>
        <name>Hinton, SR</name>
      </author>
      <author>
        <name>Hollowood, DL</name>
      </author>
      <author>
        <name>Honscheid, K</name>
      </author>
      <author>
        <name>Huterer, D</name>
      </author>
      <author>
        <name>Jain, B</name>
      </author>
      <author>
        <name>James, DJ</name>
      </author>
      <author>
        <name>Jeffrey, N</name>
      </author>
      <author>
        <name>Kasai, E</name>
      </author>
      <author>
        <name>Kelsey, L</name>
      </author>
      <author>
        <name>Kent, S</name>
      </author>
      <author>
        <name>Kessler, R</name>
      </author>
      <author>
        <name>Kim, AG</name>
        <uri>https://orcid.org/0000-0001-6315-8743</uri>
      </author>
      <author>
        <name>Kirshner, RP</name>
      </author>
      <author>
        <name>Kovacs, E</name>
      </author>
      <author>
        <name>Kuehn, K</name>
      </author>
      <author>
        <name>Lahav, O</name>
      </author>
      <author>
        <name>Lee, J</name>
      </author>
      <author>
        <name>Lee, S</name>
      </author>
      <author>
        <name>Lewis, GF</name>
      </author>
      <author>
        <name>Li, TS</name>
      </author>
      <author>
        <name>Lidman, C</name>
      </author>
      <author>
        <name>Lin, H</name>
      </author>
      <author>
        <name>Malik, U</name>
      </author>
      <author>
        <name>Marshall, JL</name>
      </author>
      <author>
        <name>Martini, P</name>
      </author>
      <author>
        <name>Mena-Fernández, J</name>
      </author>
      <author>
        <name>Menanteau, F</name>
      </author>
      <author>
        <name>Miquel, R</name>
      </author>
      <author>
        <name>Mohr, JJ</name>
      </author>
    </item>
    <item>
      <title>VERITAS and Multiwavelength Observations of the Blazar B3 2247+381 in Response to an IceCube Neutrino Alert</title>
      <link>https://escholarship.org/uc/item/2mj592qp</link>
      <description>While the sources of the diffuse astrophysical neutrino flux detected by the IceCube Neutrino Observatory are still largely unknown, one of the promising methods to improve our understanding of them is investigating the potential temporal and spatial correlations between neutrino alerts and the electromagnetic radiation from blazars. We report on the multiwavelength target-of-opportunity observations of the blazar B3 2247+381, taken in response to an IceCube multiplet alert for a cluster of muon neutrino events compatible with the source location between 2022 May 20 and 2022 November 10. B3 2247+381 was not detected with VERITAS during this time period. The source was found to be in a low-flux state in the optical, ultraviolet, and gamma-ray bands for the time interval corresponding to the neutrino event, but was detected in the hard X-ray band with NuSTAR during this period. We find the multiwavelength spectral energy distribution is described well using a simple one-zone leptonic...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/2mj592qp</guid>
      <pubDate>Thu, 17 Jul 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Acharyya, A</name>
      </author>
      <author>
        <name>Adams, CB</name>
      </author>
      <author>
        <name>Bangale, P</name>
      </author>
      <author>
        <name>Bartkoske, JT</name>
      </author>
      <author>
        <name>Benbow, W</name>
      </author>
      <author>
        <name>Buckley, JH</name>
      </author>
      <author>
        <name>Christiansen, JL</name>
      </author>
      <author>
        <name>Duerr, A</name>
      </author>
      <author>
        <name>Errando, M</name>
      </author>
      <author>
        <name>Godoy, M Escobar</name>
      </author>
      <author>
        <name>Falcone, A</name>
      </author>
      <author>
        <name>Feng, Q</name>
      </author>
      <author>
        <name>Foote, J</name>
      </author>
      <author>
        <name>Fortson, L</name>
      </author>
      <author>
        <name>Furniss, A</name>
        <uri>https://orcid.org/0000-0003-1614-1273</uri>
      </author>
      <author>
        <name>Gallagher, G</name>
      </author>
      <author>
        <name>Hanlon, W</name>
      </author>
      <author>
        <name>Hanna, D</name>
      </author>
      <author>
        <name>Hervet, O</name>
        <uri>https://orcid.org/0000-0003-3878-1677</uri>
      </author>
      <author>
        <name>Hinrichs, CE</name>
      </author>
      <author>
        <name>Hoang, J</name>
      </author>
      <author>
        <name>Holder, J</name>
      </author>
      <author>
        <name>Humensky, TB</name>
      </author>
      <author>
        <name>Jin, W</name>
      </author>
      <author>
        <name>Johnson, MN</name>
      </author>
      <author>
        <name>Kaaret, P</name>
      </author>
      <author>
        <name>Kertzman, M</name>
      </author>
      <author>
        <name>Kherlakian, M</name>
      </author>
      <author>
        <name>Kieda, D</name>
      </author>
      <author>
        <name>Kleiner, TK</name>
      </author>
      <author>
        <name>Korzoun, N</name>
      </author>
      <author>
        <name>Krennrich, F</name>
      </author>
      <author>
        <name>Kumar, S</name>
      </author>
      <author>
        <name>Lang, MJ</name>
      </author>
      <author>
        <name>Lundy, M</name>
      </author>
      <author>
        <name>McGrath, CE</name>
      </author>
      <author>
        <name>Meyer, E</name>
      </author>
      <author>
        <name>Millard, MJ</name>
      </author>
      <author>
        <name>Millis, J</name>
      </author>
      <author>
        <name>Mooney, CL</name>
      </author>
      <author>
        <name>Moriarty, P</name>
      </author>
      <author>
        <name>Mukherjee, R</name>
      </author>
      <author>
        <name>Ning, W</name>
      </author>
      <author>
        <name>O’Brien, S</name>
      </author>
      <author>
        <name>Ong, RA</name>
      </author>
      <author>
        <name>Pohl, M</name>
      </author>
      <author>
        <name>Pueschel, E</name>
      </author>
      <author>
        <name>Quinn, J</name>
      </author>
      <author>
        <name>Rabinowitz, PL</name>
      </author>
      <author>
        <name>Ragan, K</name>
      </author>
      <author>
        <name>Reynolds, PT</name>
      </author>
      <author>
        <name>Ribeiro, D</name>
      </author>
      <author>
        <name>Roache, E</name>
      </author>
      <author>
        <name>Ryan, JL</name>
      </author>
      <author>
        <name>Sadeh, I</name>
      </author>
      <author>
        <name>Sadun, AC</name>
      </author>
      <author>
        <name>Saha, L</name>
      </author>
      <author>
        <name>Santander, M</name>
      </author>
      <author>
        <name>Sembroski, GH</name>
      </author>
      <author>
        <name>Shang, R</name>
      </author>
      <author>
        <name>Splettstoesser, M</name>
      </author>
      <author>
        <name>Tak, D</name>
      </author>
      <author>
        <name>Talluri, AK</name>
      </author>
      <author>
        <name>Tucci, JV</name>
      </author>
      <author>
        <name>Valverde, J</name>
      </author>
      <author>
        <name>Williams, DA</name>
        <uri>https://orcid.org/0000-0003-2740-9714</uri>
      </author>
      <author>
        <name>Wong, SL</name>
      </author>
      <author>
        <name>Woo, J</name>
      </author>
      <author>
        <name>Abbasi, R</name>
      </author>
      <author>
        <name>Ackermann, M</name>
      </author>
      <author>
        <name>Adams, J</name>
      </author>
      <author>
        <name>Agarwalla, SK</name>
      </author>
      <author>
        <name>Aguilar, JA</name>
      </author>
      <author>
        <name>Ahlers, M</name>
      </author>
      <author>
        <name>Alameddine, JM</name>
      </author>
      <author>
        <name>Amin, NM</name>
      </author>
      <author>
        <name>Andeen, K</name>
      </author>
      <author>
        <name>Argüelles, C</name>
      </author>
      <author>
        <name>Ashida, Y</name>
      </author>
      <author>
        <name>Athanasiadou, S</name>
      </author>
      <author>
        <name>Axani, SN</name>
      </author>
      <author>
        <name>Babu, R</name>
      </author>
      <author>
        <name>Bai, X</name>
      </author>
      <author>
        <name>V., A Balagopal</name>
      </author>
      <author>
        <name>Baricevic, M</name>
      </author>
      <author>
        <name>Barwick, SW</name>
        <uri>https://orcid.org/0000-0003-2050-6714</uri>
      </author>
      <author>
        <name>Bash, S</name>
      </author>
      <author>
        <name>Basu, V</name>
      </author>
      <author>
        <name>Bay, R</name>
      </author>
      <author>
        <name>Beatty, JJ</name>
      </author>
      <author>
        <name>Tjus, J Becker</name>
      </author>
      <author>
        <name>Beise, J</name>
      </author>
      <author>
        <name>Bellenghi, C</name>
      </author>
      <author>
        <name>BenZvi, S</name>
      </author>
      <author>
        <name>Berley, D</name>
      </author>
      <author>
        <name>Bernardini, E</name>
      </author>
      <author>
        <name>Besson, DZ</name>
      </author>
      <author>
        <name>Blaufuss, E</name>
      </author>
      <author>
        <name>Bloom, L</name>
      </author>
      <author>
        <name>Blot, S</name>
      </author>
    </item>
    <item>
      <title>Giant Outer Transiting Exoplanet Mass (GOT ‘EM) Survey. V. Two Giant Planets in Kepler-511 but Only One Ran Away</title>
      <link>https://escholarship.org/uc/item/6mh6q5hg</link>
      <description>Systems hosting multiple giant planets are important laboratories for understanding planetary formation and migration processes. We present a nearly decade-long Doppler spectroscopy campaign from the HIRES instrument on the Keck-I telescope to characterize the two transiting giant planets orbiting Kepler-511 on orbits of 27 days and 297 days. The radial velocity measurements yield precise masses for both planets: 0.10 0 − 0.039 + 0.036 (2.6σ) and 0.4 4 − 0.12 + 0.11 (4σ) Jupiter masses, respectively. We use these masses to infer their bulk metallicities (i.e., metal mass fraction 0.87 ± 0.03 and 0.22 ± 0.04, respectively). Strikingly, both planets contain approximately 25-30 Earth masses of heavy elements but have very different amounts of hydrogen and helium. Envelope mass loss cannot account for this difference due to the relatively large orbital distance and mass of the inner planet. We conclude that the outer planet underwent runaway gas accretion while the inner planet did...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/6mh6q5hg</guid>
      <pubDate>Fri, 25 Apr 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Chachan, Yayaati</name>
        <uri>https://orcid.org/0000-0003-1728-8269</uri>
      </author>
      <author>
        <name>Dalba, Paul A</name>
      </author>
      <author>
        <name>Thorngren, Daniel P</name>
      </author>
      <author>
        <name>Kane, Stephen R</name>
        <uri>https://orcid.org/0000-0002-7084-0529</uri>
      </author>
      <author>
        <name>Isaacson, Howard</name>
        <uri>https://orcid.org/0000-0002-0531-1073</uri>
      </author>
      <author>
        <name>Lee, Eve J</name>
        <uri>https://orcid.org/0000-0002-1228-9820</uri>
      </author>
      <author>
        <name>Schwieterman, Edward W</name>
        <uri>https://orcid.org/0000-0002-2949-2163</uri>
      </author>
      <author>
        <name>Howard, Andrew W</name>
      </author>
      <author>
        <name>Payne, Matthew J</name>
      </author>
    </item>
    <item>
      <title>Multiwavelength constraints on the origin of a nearby repeating fast radio burst source in a globular cluster</title>
      <link>https://escholarship.org/uc/item/5v24p8hv</link>
      <description>The precise origins of fast radio bursts (FRBs) remain unknown. Multiwavelength observations of nearby FRB sources can provide important insights into the enigmatic FRB phenomenon. Here we present results from a sensitive, broadband X-ray and radio observational campaign of FRB 20200120E, the closest known extragalactic repeating FRB source (located 3.63 Mpc away in an ~10-Gyr-old globular cluster). We place deep limits on the persistent and prompt X-ray emission from FRB 20200120E, which we use to constrain possible origins for the source. We compare our results with various classes of X-ray sources, transients and FRB models. We find that FRB 20200120E is unlikely to be associated with ultraluminous X-ray bursts, magnetar-like giant flares or an SGR 1935+2154-like intermediate flare. Although other types of bright magnetar-like intermediate flares and short X-ray bursts would have been detectable from FRB 20200120E during our observations, we cannot entirely rule them out as...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/5v24p8hv</guid>
      <pubDate>Thu, 13 Feb 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Pearlman, Aaron B</name>
      </author>
      <author>
        <name>Scholz, Paul</name>
      </author>
      <author>
        <name>Bethapudi, Suryarao</name>
      </author>
      <author>
        <name>Hessels, Jason WT</name>
      </author>
      <author>
        <name>Kaspi, Victoria M</name>
      </author>
      <author>
        <name>Kirsten, Franz</name>
      </author>
      <author>
        <name>Nimmo, Kenzie</name>
      </author>
      <author>
        <name>Spitler, Laura G</name>
      </author>
      <author>
        <name>Fonseca, Emmanuel</name>
      </author>
      <author>
        <name>Meyers, Bradley W</name>
      </author>
      <author>
        <name>Stairs, Ingrid H</name>
      </author>
      <author>
        <name>Tan, Chia Min</name>
      </author>
      <author>
        <name>Bhardwaj, Mohit</name>
      </author>
      <author>
        <name>Chatterjee, Shami</name>
      </author>
      <author>
        <name>Cook, Amanda M</name>
      </author>
      <author>
        <name>Curtin, Alice P</name>
      </author>
      <author>
        <name>Dong, Fengqiu Adam</name>
      </author>
      <author>
        <name>Eftekhari, Tarraneh</name>
      </author>
      <author>
        <name>Gaensler, BM</name>
        <uri>https://orcid.org/0000-0002-3382-9558</uri>
      </author>
      <author>
        <name>Güver, Tolga</name>
      </author>
      <author>
        <name>Kaczmarek, Jane</name>
      </author>
      <author>
        <name>Leung, Calvin</name>
      </author>
      <author>
        <name>Masui, Kiyoshi W</name>
      </author>
      <author>
        <name>Michilli, Daniele</name>
      </author>
      <author>
        <name>Prince, Thomas A</name>
      </author>
      <author>
        <name>Sand, Ketan R</name>
      </author>
      <author>
        <name>Shin, Kaitlyn</name>
      </author>
      <author>
        <name>Smith, Kendrick M</name>
      </author>
      <author>
        <name>Tendulkar, Shriharsh P</name>
      </author>
    </item>
    <item>
      <title>GLEAM: The GaLactic and Extragalactic All-Sky MWA Survey</title>
      <link>https://escholarship.org/uc/item/58v375wq</link>
      <description>We describe a new low-frequency wideband radio survey of the southern sky. Observations covering 72-231MHz and Declinations south of +30° have been performed with the Murchison Widefield Array "extended" Phase I I configuration over 2018-2020 and will be processed to form data products including continuum and polarisation images and mosaics, multi-frequency catalogues, transient search data, and ionospheric measurements. From a pilot field described in this work, we publish an initial data release covering 1,447 deg&lt;sup&gt;2&lt;/sup&gt; over 4 h≤ RA≤ 13 h, -32.7° ≤ Dec ≤ -20.7°. We process twenty frequency bands sampling 72-231 MHz, with a resolution of 2'-45″, and produce a wideband source-finding image across 170-231MHz with a root-mean-square noise of 1.27 ± 0.15 mJy beam&lt;sup&gt;-1&lt;/sup&gt;. Source-finding yields 79,124 components, of which 71,320 are fitted spectrally. The catalogue has a completeness of 98% at ~ 50 mJy, and a reliability of 98.2% at 5&lt;i&gt;σ&lt;/i&gt; rising to 99.7% at 7&lt;i&gt;σ&lt;/i&gt;....</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/58v375wq</guid>
      <pubDate>Fri, 6 Dec 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Wayth, RB</name>
      </author>
      <author>
        <name>Lenc, E</name>
      </author>
      <author>
        <name>Bell, ME</name>
      </author>
      <author>
        <name>Callingham, JR</name>
      </author>
      <author>
        <name>Dwarakanath, KS</name>
      </author>
      <author>
        <name>Franzen, TMO</name>
      </author>
      <author>
        <name>For, B-Q</name>
      </author>
      <author>
        <name>Gaensler, B</name>
        <uri>https://orcid.org/0000-0002-3382-9558</uri>
      </author>
      <author>
        <name>Hancock, P</name>
      </author>
      <author>
        <name>Hindson, L</name>
      </author>
      <author>
        <name>Hurley-Walker, N</name>
      </author>
      <author>
        <name>Jackson, CA</name>
      </author>
      <author>
        <name>Johnston-Hollitt, M</name>
      </author>
      <author>
        <name>Kapińska, AD</name>
      </author>
      <author>
        <name>McKinley, B</name>
      </author>
      <author>
        <name>Morgan, J</name>
      </author>
      <author>
        <name>Offringa, AR</name>
      </author>
      <author>
        <name>Procopio, P</name>
      </author>
      <author>
        <name>Staveley-Smith, L</name>
      </author>
      <author>
        <name>Wu, C</name>
      </author>
      <author>
        <name>Zheng, Q</name>
      </author>
      <author>
        <name>Trott, CM</name>
      </author>
      <author>
        <name>Bernardi, G</name>
      </author>
      <author>
        <name>Bowman, JD</name>
      </author>
      <author>
        <name>Briggs, F</name>
      </author>
      <author>
        <name>Cappallo, RJ</name>
      </author>
      <author>
        <name>Corey, BE</name>
      </author>
      <author>
        <name>Deshpande, AA</name>
      </author>
      <author>
        <name>Emrich, D</name>
      </author>
      <author>
        <name>Goeke, R</name>
      </author>
      <author>
        <name>Greenhill, LJ</name>
      </author>
      <author>
        <name>Hazelton, BJ</name>
      </author>
      <author>
        <name>Kaplan, DL</name>
      </author>
      <author>
        <name>Kasper, JC</name>
      </author>
      <author>
        <name>Kratzenberg, E</name>
      </author>
      <author>
        <name>Lonsdale, CJ</name>
      </author>
      <author>
        <name>Lynch, MJ</name>
      </author>
      <author>
        <name>McWhirter, SR</name>
      </author>
      <author>
        <name>Mitchell, DA</name>
      </author>
      <author>
        <name>Morales, MF</name>
      </author>
      <author>
        <name>Morgan, E</name>
      </author>
      <author>
        <name>Oberoi, D</name>
      </author>
      <author>
        <name>Ord, SM</name>
      </author>
      <author>
        <name>Prabu, T</name>
      </author>
      <author>
        <name>Rogers, AEE</name>
      </author>
      <author>
        <name>Roshi, A</name>
      </author>
      <author>
        <name>Shankar, N Udaya</name>
      </author>
      <author>
        <name>Srivani, KS</name>
      </author>
      <author>
        <name>Subrahmanyan, R</name>
      </author>
      <author>
        <name>Tingay, SJ</name>
      </author>
      <author>
        <name>Waterson, M</name>
      </author>
      <author>
        <name>Webster, RL</name>
      </author>
      <author>
        <name>Whitney, AR</name>
      </author>
      <author>
        <name>Williams, A</name>
      </author>
      <author>
        <name>Williams, CL</name>
      </author>
    </item>
    <item>
      <title>A trail of dark-matter-free galaxies from a bullet-dwarf collision</title>
      <link>https://escholarship.org/uc/item/6nv5f7t1</link>
      <description>The ultra-diffuse galaxies DF2 and DF4 in the NGC 1052 group share several unusual properties: they both have large sizes1, rich populations of overluminous and large globular clusters2–6, and very low velocity dispersions that indicate little or no dark matter7–10. It has been suggested that these galaxies were formed in the aftermath of high-velocity collisions of gas-rich galaxies11–13, events that resemble the collision that created the bullet cluster14 but on much smaller scales. The gas separates from the dark matter in the collision and subsequent star formation leads to the formation of one or more dark-matter-free galaxies12. Here we show that the present-day line-of-sight distances and radial velocities of DF2 and DF4 are consistent with their joint formation in the aftermath of a single bullet-dwarf collision, around eight billion years ago. Moreover, we find that DF2 and DF4 are part of an apparent linear substructure of seven to eleven large, low-luminosity objects....</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/6nv5f7t1</guid>
      <pubDate>Fri, 11 Oct 2024 00:00:00 +0000</pubDate>
      <author>
        <name>van Dokkum, Pieter</name>
      </author>
      <author>
        <name>Shen, Zili</name>
      </author>
      <author>
        <name>Keim, Michael A</name>
      </author>
      <author>
        <name>Trujillo-Gomez, Sebastian</name>
      </author>
      <author>
        <name>Danieli, Shany</name>
      </author>
      <author>
        <name>Dutta Chowdhury, Dhruba</name>
      </author>
      <author>
        <name>Abraham, Roberto</name>
      </author>
      <author>
        <name>Conroy, Charlie</name>
      </author>
      <author>
        <name>Kruijssen, JM Diederik</name>
      </author>
      <author>
        <name>Nagai, Daisuke</name>
      </author>
      <author>
        <name>Romanowsky, Aaron</name>
        <uri>https://orcid.org/0000-0003-2473-0369</uri>
      </author>
    </item>
    <item>
      <title>Laboratory demonstration of optimal identification and control of tip-tilt systems</title>
      <link>https://escholarship.org/uc/item/827319f9</link>
      <description>Laboratory demonstration of optimal identification and control of tip-tilt systems</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/827319f9</guid>
      <pubDate>Sat, 20 Jul 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Sengupta, Aditya R</name>
      </author>
      <author>
        <name>Gerard, Benjamin L</name>
      </author>
      <author>
        <name>Dillon, Daren</name>
      </author>
      <author>
        <name>van Kooten, Maaike</name>
      </author>
      <author>
        <name>Gavel, Donald</name>
      </author>
      <author>
        <name>Jensen-Clem, Rebecca</name>
      </author>
    </item>
    <item>
      <title>Teaching and Learning During A Pandemic: How one Graduate Community Psychology Class Quickly Incorporated Healing Justice Into Our Practices</title>
      <link>https://escholarship.org/uc/item/11k6n2tx</link>
      <description>In this first-person account, we describe the changes we made to align our graduate student-level community psychology class with a healing justice model. We undertook this intervention because the class started in March, at the beginning of the COVID-19 pandemic stay-at-home directive in our region. We describe the facets of a healing justice model, which promotes radical healing and collective action in a trauma-informed environment. We then discuss the changes we made to the class to better align with healing justice, including how enrolled students (i.e., co-authors) experienced the process of the course (e.g., reworking the syllabus, starting class with check-ins and an exercise to engage our parasympathetic nervous systems), as well as the content of the course (e.g., service projects to support people who are undocumented, unhoused, or minoritized in other ways; photovoice). We end with implications for teaching community psychology, including the importance of universal...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/11k6n2tx</guid>
      <pubDate>Fri, 19 Jul 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Langhout, Regina Day</name>
        <uri>https://orcid.org/0000-0001-9607-8539</uri>
      </author>
      <author>
        <name>Ramirez, Daniel Rodriguez</name>
      </author>
      <author>
        <name>Vaccarino‐Ruiz, S Sylvane</name>
      </author>
      <author>
        <name>Blanco, Valeria Alonso</name>
      </author>
      <author>
        <name>Quinteros, Katherine</name>
      </author>
      <author>
        <name>Copulsky, Daniel</name>
      </author>
      <author>
        <name>Lopezzi, Miguel A</name>
      </author>
    </item>
    <item>
      <title>Search for Ultraheavy Dark Matter from Observations of Dwarf Spheroidal Galaxies with VERITAS</title>
      <link>https://escholarship.org/uc/item/7fc5q0p2</link>
      <description>Dark matter is a key piece of the current cosmological scenario, with weakly interacting massive particles (WIMPs) a leading dark matter candidate. WIMPs have not been detected in their conventional parameter space (100 GeV ≲M χ ≲ 100 TeV), a mass range accessible with current Imaging Atmospheric Cherenkov Telescopes. As ultraheavy dark matter (UHDM; M χ ≳ 100 TeV) has been suggested as an underexplored alternative to the WIMP paradigm, we search for an indirect dark matter annihilation signal in a higher mass range (up to 30 PeV) with the VERITAS γ-ray observatory. With 216 hr of observations of four dwarf spheroidal galaxies, we perform an unbinned likelihood analysis. We find no evidence of a γ-ray signal from UHDM annihilation above the background fluctuation for any individual dwarf galaxy nor for a joint-fit analysis, and consequently constrain the velocity-weighted annihilation cross section of UHDM for dark matter particle masses between 1 TeV and 30 PeV. We additionally...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/7fc5q0p2</guid>
      <pubDate>Wed, 10 Jul 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Acharyya, A</name>
      </author>
      <author>
        <name>Archer, A</name>
      </author>
      <author>
        <name>Bangale, P</name>
      </author>
      <author>
        <name>Bartkoske, JT</name>
      </author>
      <author>
        <name>Batista, P</name>
      </author>
      <author>
        <name>Baumgart, M</name>
      </author>
      <author>
        <name>Benbow, W</name>
      </author>
      <author>
        <name>Buckley, JH</name>
      </author>
      <author>
        <name>Falcone, A</name>
      </author>
      <author>
        <name>Feng, Q</name>
      </author>
      <author>
        <name>Finley, JP</name>
      </author>
      <author>
        <name>Foote, GM</name>
      </author>
      <author>
        <name>Fortson, L</name>
      </author>
      <author>
        <name>Furniss, A</name>
        <uri>https://orcid.org/0000-0003-1614-1273</uri>
      </author>
      <author>
        <name>Gallagher, G</name>
      </author>
      <author>
        <name>Hanlon, WF</name>
      </author>
      <author>
        <name>Hervet, O</name>
        <uri>https://orcid.org/0000-0003-3878-1677</uri>
      </author>
      <author>
        <name>Hoang, J</name>
      </author>
      <author>
        <name>Holder, J</name>
      </author>
      <author>
        <name>Humensky, TB</name>
      </author>
      <author>
        <name>Jin, W</name>
      </author>
      <author>
        <name>Kaaret, P</name>
      </author>
      <author>
        <name>Kertzman, M</name>
      </author>
      <author>
        <name>Kherlakian, M</name>
      </author>
      <author>
        <name>Kieda, D</name>
      </author>
      <author>
        <name>Kleiner, TK</name>
      </author>
      <author>
        <name>Korzoun, N</name>
      </author>
      <author>
        <name>Krennrich, F</name>
      </author>
      <author>
        <name>Lang, MJ</name>
      </author>
      <author>
        <name>Lundy, M</name>
      </author>
      <author>
        <name>Maier, G</name>
      </author>
      <author>
        <name>McGrath, CE</name>
      </author>
      <author>
        <name>Moriarty, P</name>
      </author>
      <author>
        <name>O’Brien, S</name>
      </author>
      <author>
        <name>Ong, RA</name>
      </author>
      <author>
        <name>Pfrang, K</name>
      </author>
      <author>
        <name>Pohl, M</name>
      </author>
      <author>
        <name>Pueschel, E</name>
      </author>
      <author>
        <name>Quinn, J</name>
      </author>
      <author>
        <name>Ragan, K</name>
      </author>
      <author>
        <name>Reynolds, PT</name>
      </author>
      <author>
        <name>Roache, E</name>
      </author>
      <author>
        <name>Rodd, NL</name>
        <uri>https://orcid.org/0000-0003-3472-7606</uri>
      </author>
      <author>
        <name>Ryan, JL</name>
      </author>
      <author>
        <name>Sadeh, I</name>
      </author>
      <author>
        <name>Saha, L</name>
      </author>
      <author>
        <name>Santander, M</name>
      </author>
      <author>
        <name>Sembroski, GH</name>
      </author>
      <author>
        <name>Shang, R</name>
      </author>
      <author>
        <name>Splettstoesser, M</name>
      </author>
      <author>
        <name>Tak, D</name>
      </author>
      <author>
        <name>Tucci, JV</name>
      </author>
      <author>
        <name>Vassiliev, VV</name>
      </author>
      <author>
        <name>Williams, DA</name>
        <uri>https://orcid.org/0000-0003-2740-9714</uri>
      </author>
    </item>
    <item>
      <title>GTC Follow-up Observations of Very Metal-poor Star Candidates from DESI</title>
      <link>https://escholarship.org/uc/item/7m06d2jp</link>
      <description>The observations from the Dark Energy Spectroscopic Instrument (DESI) will significantly increase the numbers of known extremely metal-poor stars by a factor of ∼10, improving the sample statistics to study the early chemical evolution of the Milky Way and the nature of the first stars. In this paper we report follow-up observations with high signal-to-noise ratio of nine metal-poor stars identified during the DESI commissioning with the Optical System for Imaging and Low-Resolution Integrated Spectroscopy (OSIRIS) instrument on the 10.4 m Gran Telescopio Canarias. The analysis of the data using a well-vetted methodology confirms the quality of the DESI spectra and the performance of the pipelines developed for the data reduction and analysis of DESI data.</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/7m06d2jp</guid>
      <pubDate>Thu, 30 May 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Prieto, Carlos Allende</name>
      </author>
      <author>
        <name>Aguado, David S</name>
      </author>
      <author>
        <name>Hernández, Jonay I González</name>
      </author>
      <author>
        <name>Rebolo, Rafael</name>
      </author>
      <author>
        <name>Najita, Joan</name>
      </author>
      <author>
        <name>Manser, Christopher J</name>
      </author>
      <author>
        <name>Rockosi, Constance</name>
      </author>
      <author>
        <name>Slepian, Zachary</name>
      </author>
      <author>
        <name>Mezcua, Mar</name>
      </author>
      <author>
        <name>Valluri, Monica</name>
      </author>
      <author>
        <name>Ezzeddine, Rana</name>
      </author>
      <author>
        <name>Koposov, Sergey E</name>
      </author>
      <author>
        <name>Cooper, Andrew P</name>
      </author>
      <author>
        <name>Dey, Arjun</name>
      </author>
      <author>
        <name>Gänsicke, Boris T</name>
      </author>
      <author>
        <name>Li, Ting S</name>
      </author>
      <author>
        <name>Cunha, Katia</name>
      </author>
      <author>
        <name>Zou, Siwei</name>
      </author>
      <author>
        <name>Aguilar, Jessica Nicole</name>
      </author>
      <author>
        <name>Ahlen, Steven</name>
      </author>
      <author>
        <name>Brooks, David</name>
      </author>
      <author>
        <name>Claybaugh, Todd</name>
      </author>
      <author>
        <name>Cole, Shaun</name>
      </author>
      <author>
        <name>Eftekharzadeh, Sarah</name>
      </author>
      <author>
        <name>Fanning, Kevin</name>
      </author>
      <author>
        <name>Forero-Romero, Jaime</name>
      </author>
      <author>
        <name>Gontcho, Satya Gontcho A</name>
      </author>
      <author>
        <name>Honscheid, Klaus</name>
      </author>
      <author>
        <name>Jablonka, Pascale</name>
      </author>
      <author>
        <name>Kehoe, Robert</name>
      </author>
      <author>
        <name>Kisner, Theodore</name>
      </author>
      <author>
        <name>Landriau, Martin</name>
        <uri>https://orcid.org/0000-0003-1838-8528</uri>
      </author>
      <author>
        <name>de la Macorra, Axel</name>
      </author>
      <author>
        <name>Meisner, Aaron</name>
      </author>
      <author>
        <name>Miquel, Ramón</name>
      </author>
      <author>
        <name>Moustakas, John</name>
      </author>
      <author>
        <name>Nie, Jundan</name>
      </author>
      <author>
        <name>Poppett, Claire</name>
      </author>
      <author>
        <name>Prada, Francisco</name>
      </author>
      <author>
        <name>Rezaie, Mehdi</name>
      </author>
      <author>
        <name>Rossi, Graziano</name>
      </author>
      <author>
        <name>Sánchez, Eusebio</name>
      </author>
      <author>
        <name>Schubnell, Michael</name>
      </author>
      <author>
        <name>Sharples, Ray</name>
      </author>
      <author>
        <name>Siudek, Malgorzata</name>
      </author>
      <author>
        <name>Smith, Verne V</name>
      </author>
      <author>
        <name>Tarlé, Gregory</name>
      </author>
      <author>
        <name>Vincenzo, Fiorenzo</name>
      </author>
      <author>
        <name>Weaver, Benjamin Alan</name>
      </author>
      <author>
        <name>Zhou, Zhimin</name>
      </author>
      <author>
        <name>Zou, Hu</name>
      </author>
    </item>
    <item>
      <title>Giant Outer Transiting Exoplanet Mass (GOT ‘EM) Survey. IV. Long-term Doppler Spectroscopy for 11 Stars Thought to Host Cool Giant Exoplanets</title>
      <link>https://escholarship.org/uc/item/8xr2s1dv</link>
      <description>Discovering and characterizing exoplanets at the outer edge of the transit method’s sensitivity has proven challenging owing to geometric biases and the practical difficulties associated with acquiring long observational baselines. Nonetheless, a sample of giant exoplanets on orbits longer than 100 days has been identified by transit hunting missions. We present long-term Doppler spectroscopy for 11 such systems with observation baselines spanning a few years to a decade. We model these radial velocity observations jointly with transit photometry to provide initial characterizations of these objects and the systems in which they exist. Specifically, we make new precise mass measurements for four long-period giant exoplanets (Kepler-111 c, Kepler-553 c, Kepler-849 b, and PH-2 b), we place new upper limits on mass for four others (Kepler-421 b, KOI-1431.01, Kepler-1513 b, and Kepler-952 b), and we show that several confirmed planets are in fact not planetary at all. We present these...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/8xr2s1dv</guid>
      <pubDate>Thu, 23 May 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Dalba, Paul A</name>
      </author>
      <author>
        <name>Kane, Stephen R</name>
        <uri>https://orcid.org/0000-0002-7084-0529</uri>
      </author>
      <author>
        <name>Isaacson, Howard</name>
        <uri>https://orcid.org/0000-0002-0531-1073</uri>
      </author>
      <author>
        <name>Fulton, Benjamin</name>
      </author>
      <author>
        <name>Howard, Andrew W</name>
      </author>
      <author>
        <name>Schwieterman, Edward W</name>
        <uri>https://orcid.org/0000-0002-2949-2163</uri>
      </author>
      <author>
        <name>Thorngren, Daniel P</name>
      </author>
      <author>
        <name>Fortney, Jonathan</name>
        <uri>https://orcid.org/0000-0002-9843-4354</uri>
      </author>
      <author>
        <name>Vowell, Noah</name>
      </author>
      <author>
        <name>Beard, Corey</name>
      </author>
      <author>
        <name>Blunt, Sarah</name>
      </author>
      <author>
        <name>Brinkman, Casey L</name>
      </author>
      <author>
        <name>Chontos, Ashley</name>
      </author>
      <author>
        <name>Dai, Fei</name>
      </author>
      <author>
        <name>Giacalone, Steven</name>
      </author>
      <author>
        <name>Hill, Michelle L</name>
      </author>
      <author>
        <name>Kosiarek, Molly</name>
      </author>
      <author>
        <name>Lubin, Jack</name>
      </author>
      <author>
        <name>Mayo, Andrew W</name>
      </author>
      <author>
        <name>Močnik, Teo</name>
      </author>
      <author>
        <name>Murphy, Joseph M Akana</name>
      </author>
      <author>
        <name>Petigura, Erik A</name>
      </author>
      <author>
        <name>Rice, Malena</name>
      </author>
      <author>
        <name>Rubenzahl, Ryan A</name>
      </author>
      <author>
        <name>Van Zandt, Judah</name>
      </author>
      <author>
        <name>Weiss, Lauren M</name>
      </author>
      <author>
        <name>Dragomir, Diana</name>
      </author>
      <author>
        <name>Kipping, David</name>
      </author>
      <author>
        <name>Payne, Matthew J</name>
      </author>
      <author>
        <name>Roy, Arpita</name>
      </author>
      <author>
        <name>Teachey, Alex</name>
      </author>
      <author>
        <name>Villanueva, Steven</name>
      </author>
    </item>
    <item>
      <title>Reimagining leadership through the everyday resistance of faculty of color.</title>
      <link>https://escholarship.org/uc/item/33q2b7z3</link>
      <description>Reimagining leadership through the everyday resistance of faculty of color.</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/33q2b7z3</guid>
      <pubDate>Tue, 26 Mar 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Quinteros, Katherine N</name>
      </author>
      <author>
        <name>Covarrubias, Rebecca</name>
      </author>
    </item>
    <item>
      <title>The intrinsic alignment of red galaxies in DES Y1 redMaPPer galaxy clusters</title>
      <link>https://escholarship.org/uc/item/2zx192jq</link>
      <description>ABSTRACT Clusters of galaxies trace the most non-linear peaks in the cosmic density field. The weak gravitational lensing of background galaxies by clusters can allow us to infer their masses. However, galaxies associated with the local environment of the cluster can also be intrinsically aligned due to the local tidal gradient, contaminating any cosmology derived from the lensing signal. We measure this intrinsic alignment in Dark Energy Survey (DES) Year 1 redMaPPer clusters. We find evidence of a non-zero mean radial alignment of galaxies within clusters between redshifts 0.1–0.7. We find a significant systematic in the measured ellipticities of cluster satellite galaxies that we attribute to the central galaxy flux and other intracluster light. We attempt to correct this signal, and fit a simple model for intrinsic alignment amplitude (AIA) to the measurement, finding AIA&amp;nbsp;= 0.15&amp;nbsp;±&amp;nbsp;0.04, when excluding data near the edge of the cluster. We find a significantly...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/2zx192jq</guid>
      <pubDate>Wed, 14 Feb 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Zhou, C</name>
        <uri>https://orcid.org/0000-0002-2897-6326</uri>
      </author>
      <author>
        <name>Tong, A</name>
      </author>
      <author>
        <name>Troxel, MA</name>
      </author>
      <author>
        <name>Blazek, J</name>
      </author>
      <author>
        <name>Lin, C</name>
      </author>
      <author>
        <name>Bacon, D</name>
      </author>
      <author>
        <name>Bleem, L</name>
      </author>
      <author>
        <name>Chang, C</name>
      </author>
      <author>
        <name>Costanzi, M</name>
      </author>
      <author>
        <name>DeRose, J</name>
      </author>
      <author>
        <name>Dietrich, JP</name>
      </author>
      <author>
        <name>Drlica-Wagner, A</name>
      </author>
      <author>
        <name>Gruen, D</name>
      </author>
      <author>
        <name>Gruendl, RA</name>
      </author>
      <author>
        <name>Hoyle, B</name>
      </author>
      <author>
        <name>Jarvis, M</name>
      </author>
      <author>
        <name>MacCrann, N</name>
      </author>
      <author>
        <name>Mawdsley, B</name>
      </author>
      <author>
        <name>McClintock, T</name>
      </author>
      <author>
        <name>Melchior, P</name>
      </author>
      <author>
        <name>Prat, J</name>
      </author>
      <author>
        <name>Pujol, A</name>
      </author>
      <author>
        <name>Rozo, E</name>
      </author>
      <author>
        <name>Rykoff, ES</name>
      </author>
      <author>
        <name>Samuroff, S</name>
      </author>
      <author>
        <name>Sheldon, E</name>
      </author>
      <author>
        <name>Shin, T</name>
      </author>
      <author>
        <name>Rosell, A Carnero</name>
      </author>
      <author>
        <name>Yanny, B</name>
      </author>
      <author>
        <name>Sánchez, C</name>
      </author>
      <author>
        <name>Tucker, DL</name>
      </author>
      <author>
        <name>Sevilla-Noarbe, I</name>
      </author>
      <author>
        <name>Zuntz, J</name>
      </author>
      <author>
        <name>Varga, TN</name>
      </author>
      <author>
        <name>Zhang, Y</name>
      </author>
      <author>
        <name>Alves, O</name>
      </author>
      <author>
        <name>Amon, A</name>
      </author>
      <author>
        <name>Bertin, E</name>
      </author>
      <author>
        <name>Brooks, D</name>
      </author>
      <author>
        <name>Burke, DL</name>
      </author>
      <author>
        <name>Kind, M Carrasco</name>
      </author>
      <author>
        <name>da Costa, LN</name>
      </author>
      <author>
        <name>Davis, TM</name>
      </author>
      <author>
        <name>De Vicente, J</name>
      </author>
      <author>
        <name>Desai, S</name>
      </author>
      <author>
        <name>Diehl, HT</name>
      </author>
      <author>
        <name>Doel, P</name>
      </author>
      <author>
        <name>Everett, S</name>
      </author>
      <author>
        <name>Ferrero, I</name>
      </author>
      <author>
        <name>Flaugher, B</name>
      </author>
      <author>
        <name>Frieman, J</name>
      </author>
      <author>
        <name>Gerdes, DW</name>
      </author>
      <author>
        <name>Gutierrez, G</name>
      </author>
      <author>
        <name>Hinton, SR</name>
      </author>
      <author>
        <name>Hollowood, DL</name>
      </author>
      <author>
        <name>Honscheid, K</name>
      </author>
      <author>
        <name>James, DJ</name>
      </author>
      <author>
        <name>Jeltema, T</name>
      </author>
      <author>
        <name>Kuehn, K</name>
      </author>
      <author>
        <name>Lahav, O</name>
      </author>
      <author>
        <name>Lima, M</name>
      </author>
      <author>
        <name>Marshall, JL</name>
      </author>
      <author>
        <name>Mena-Fernández, J</name>
      </author>
      <author>
        <name>Menanteau, F</name>
      </author>
      <author>
        <name>Miquel, R</name>
      </author>
      <author>
        <name>Palmese, A</name>
      </author>
      <author>
        <name>Paz-Chinchón, F</name>
      </author>
      <author>
        <name>Pieres, A</name>
      </author>
      <author>
        <name>Malagón, AA Plazas</name>
      </author>
      <author>
        <name>Porredon, A</name>
      </author>
      <author>
        <name>Raveri, M</name>
      </author>
      <author>
        <name>Romer, AK</name>
      </author>
      <author>
        <name>Sanchez, E</name>
      </author>
      <author>
        <name>Smith, M</name>
      </author>
      <author>
        <name>Soares-Santos, M</name>
      </author>
      <author>
        <name>Suchyta, E</name>
      </author>
      <author>
        <name>Swanson, MEC</name>
      </author>
      <author>
        <name>Tarle, G</name>
      </author>
      <author>
        <name>To, C</name>
      </author>
      <author>
        <name>Weaverdyck, N</name>
      </author>
      <author>
        <name>Weller, J</name>
      </author>
      <author>
        <name>Wiseman, P</name>
      </author>
    </item>
    <item>
      <title>Multidimensional Radiation Hydrodynamics Simulations of Pulsational Pair-instability Supernovae</title>
      <link>https://escholarship.org/uc/item/8cx2g916</link>
      <description>Stars with masses of 80–130 M ⊙ can encounter pulsational pair-instability at the end of their lives, which triggers consecutive episodes of explosive burning that eject multiple massive shells. Collisions between these shells produce bright transients known as pulsational pair-instability supernovae (PPI SNe) that may explain some extreme supernovae. In this paper, we present the first 2D and 3D radiation hydrodynamics simulations of PPI SNe with the CASTRO code. Radiative cooling causes the collided shells to evolve into thin, dense structures with hot spots that can enhance the peak luminosity of the SN by factors of 2–3. The light curve peaks at 1.9–2.1 × 1043 erg s−1 for 50 days and then plateaus at 2–3 × 1042 erg s−1 for 200 days, depending on the viewing angle. The presence of 12C and 16O and the absence of 28Si and 56Fe in its spectra can uniquely identify this transient as a PPI SN in follow-up observations. Our models suggest that multidimensional radiation hydrodynamics...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/8cx2g916</guid>
      <pubDate>Fri, 12 Jan 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Chen, Ke-Jung</name>
      </author>
      <author>
        <name>Whalen, Daniel J</name>
      </author>
      <author>
        <name>Woosley, SE</name>
      </author>
      <author>
        <name>Zhang, Weiqun</name>
        <uri>https://orcid.org/0000-0001-8092-1974</uri>
      </author>
    </item>
    <item>
      <title>The TESS-Keck Survey. XVI. Mass Measurements for 12 Planets in Eight Systems</title>
      <link>https://escholarship.org/uc/item/11n957n7</link>
      <description>With JWST’s successful deployment and unexpectedly high fuel reserves, measuring the masses of sub-Neptunes transiting bright, nearby stars will soon become the bottleneck for characterizing the atmospheres of small exoplanets via transmission spectroscopy. Using a carefully curated target list and observations from more than 2 yr of APF-Levy and Keck-HIRES Doppler monitoring, the TESS-Keck Survey is working toward alleviating this pressure. Here we present mass measurements for 11 transiting planets in eight systems that are particularly suited to atmospheric follow-up with JWST. We also report the discovery and confirmation of a temperate super-Jovian-mass planet on a moderately eccentric orbit. The sample of eight host stars, which includes one subgiant, spans early-K to late-F spectral types (T eff = 5200-6200 K). We homogeneously derive planet parameters using a joint photometry and radial velocity modeling framework, discuss the planets’ possible bulk compositions, and comment...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/11n957n7</guid>
      <pubDate>Fri, 10 Nov 2023 00:00:00 +0000</pubDate>
      <author>
        <name>Murphy, Joseph M Akana</name>
      </author>
      <author>
        <name>Batalha, Natalie M</name>
      </author>
      <author>
        <name>Scarsdale, Nicholas</name>
      </author>
      <author>
        <name>Isaacson, Howard</name>
        <uri>https://orcid.org/0000-0002-0531-1073</uri>
      </author>
      <author>
        <name>Ciardi, David R</name>
      </author>
      <author>
        <name>Gonzales, Erica J</name>
      </author>
      <author>
        <name>Giacalone, Steven</name>
      </author>
      <author>
        <name>Twicken, Joseph D</name>
      </author>
      <author>
        <name>Dattilo, Anne</name>
      </author>
      <author>
        <name>Fetherolf, Tara</name>
      </author>
      <author>
        <name>Rubenzahl, Ryan A</name>
      </author>
      <author>
        <name>Crossfield, Ian JM</name>
      </author>
      <author>
        <name>Dressing, Courtney D</name>
        <uri>https://orcid.org/0000-0001-8189-0233</uri>
      </author>
      <author>
        <name>Fulton, Benjamin</name>
      </author>
      <author>
        <name>Howard, Andrew W</name>
      </author>
      <author>
        <name>Huber, Daniel</name>
      </author>
      <author>
        <name>Kane, Stephen R</name>
        <uri>https://orcid.org/0000-0002-7084-0529</uri>
      </author>
      <author>
        <name>Petigura, Erik A</name>
      </author>
      <author>
        <name>Robertson, Paul</name>
      </author>
      <author>
        <name>Roy, Arpita</name>
      </author>
      <author>
        <name>Weiss, Lauren M</name>
      </author>
      <author>
        <name>Beard, Corey</name>
      </author>
      <author>
        <name>Chontos, Ashley</name>
      </author>
      <author>
        <name>Dai, Fei</name>
      </author>
      <author>
        <name>Rice, Malena</name>
      </author>
      <author>
        <name>Van Zandt, Judah</name>
      </author>
      <author>
        <name>Lubin, Jack</name>
      </author>
      <author>
        <name>Blunt, Sarah</name>
      </author>
      <author>
        <name>Polanski, Alex S</name>
      </author>
      <author>
        <name>Behmard, Aida</name>
      </author>
      <author>
        <name>Dalba, Paul A</name>
      </author>
      <author>
        <name>Hill, Michelle L</name>
      </author>
      <author>
        <name>Rosenthal, Lee J</name>
      </author>
      <author>
        <name>Brinkman, Casey L</name>
      </author>
      <author>
        <name>Mayo, Andrew W</name>
      </author>
      <author>
        <name>Turtelboom, Emma V</name>
      </author>
      <author>
        <name>Angelo, Isabel</name>
      </author>
      <author>
        <name>Močnik, Teo</name>
      </author>
      <author>
        <name>MacDougall, Mason G</name>
      </author>
      <author>
        <name>Pidhorodetska, Daria</name>
      </author>
      <author>
        <name>Tyler, Dakotah</name>
        <uri>https://orcid.org/0000-0003-0298-4667</uri>
      </author>
      <author>
        <name>Kosiarek, Molly R</name>
      </author>
      <author>
        <name>Holcomb, Rae</name>
      </author>
      <author>
        <name>Louden, Emma M</name>
      </author>
      <author>
        <name>Hirsch, Lea A</name>
      </author>
      <author>
        <name>Gilbert, Emily A</name>
      </author>
      <author>
        <name>Anderson, Jay</name>
      </author>
      <author>
        <name>Valenti, Jeff A</name>
      </author>
    </item>
    <item>
      <title>Onthophagus taurus Increases Soil Microbes Associated with Nutrient Cycling in California Pastureland Soils</title>
      <link>https://escholarship.org/uc/item/2wz4q4tf</link>
      <description>Onthophagus taurus Increases Soil Microbes Associated with Nutrient Cycling in California Pastureland Soils</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/2wz4q4tf</guid>
      <pubDate>Mon, 30 Oct 2023 00:00:00 +0000</pubDate>
      <author>
        <name>Lipton, Suzanne</name>
      </author>
      <author>
        <name>Meyer, Rachel S</name>
      </author>
      <author>
        <name>Richardson, Greg</name>
      </author>
      <author>
        <name>Philpott, Stacy M</name>
      </author>
    </item>
    <item>
      <title>Atmospheric Retrieval of L Dwarfs: Benchmarking Results and Characterizing the Young Planetary Mass Companion HD 106906 b in the Near-infrared</title>
      <link>https://escholarship.org/uc/item/6vc8h47h</link>
      <description>Abstract: 

               We present model constraints on the atmospheric structure of HD 106906 b, a planetary-mass companion orbiting at a ∼700 au projected separation around a 15 Myr old stellar binary, using the APOLLO retrieval code on spectral data spanning 1.1–2.5 μm. C/O ratios can provide evidence for companion formation pathways, as such pathways are ambiguous both at wide separations and at star-to-companion mass ratios in the overlap between the distributions of planets and brown dwarfs. We benchmark our code against an existing retrieval of the field L dwarf 2MASSW J2224–0158, returning a C/O ratio consistent with previous fits to the same JHK
                  
                     s
                   data, but disagreeing in the thermal structure, cloud properties, and atmospheric scale height. For HD 106906 b, we retrieve C/O 
                     


                     
                        =
                        
                           
        ...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/6vc8h47h</guid>
      <pubDate>Thu, 26 Oct 2023 00:00:00 +0000</pubDate>
      <author>
        <name>Adams, Arthur D</name>
      </author>
      <author>
        <name>Meyer, Michael R</name>
      </author>
      <author>
        <name>Howe, Alex R</name>
      </author>
      <author>
        <name>Burningham, Ben</name>
      </author>
      <author>
        <name>Daemgen, Sebastian</name>
      </author>
      <author>
        <name>Fortney, Jonathan</name>
        <uri>https://orcid.org/0000-0002-9843-4354</uri>
      </author>
      <author>
        <name>Line, Mike</name>
      </author>
      <author>
        <name>Marley, Mark</name>
      </author>
      <author>
        <name>Quanz, Sascha P</name>
      </author>
      <author>
        <name>Todorov, Kamen</name>
      </author>
    </item>
    <item>
      <title>The detection of intergalactic H α emission from the Slug Nebula at z ∼ 2.3</title>
      <link>https://escholarship.org/uc/item/8v69h64n</link>
      <description>The Slug Nebula is one of the largest and most luminous Lyman-alpha (LyA)
nebulae discovered to date, extending over 450 kiloparsecs (kpc) around the
bright quasar UM287 at z=2.283. Characterized by high surface brightnesses over
intergalactic scales, its LyA emission may either trace high-density ionized
gas ("clumps") or large column densities of neutral material. To distinguish
between these two possibilities, information from a non-resonant line such as
Halpha is crucial. Therefore, we analyzed a deep MOSFIRE observation of one of
the brightest LyA emitting regions in the Slug Nebula with the goal of
detecting associated Halpha emission. We also obtained a deep, moderate
resolution LyA spectrum of the nearby brightest region of the Slug. We detected
an Halpha flux of F_(Halpha)= 2.62 +/- 0.47 x 10^-17 erg/cm^2/s
(SB_(Halpha)=2.70 +/- 0.48 x 10^-18 erg/cm^2/s/sq") at the expected spatial and
spectral location. Combining the Halpha detection with its corresponding LyA
flux (determined...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/8v69h64n</guid>
      <pubDate>Thu, 14 Sep 2023 00:00:00 +0000</pubDate>
      <author>
        <name>Leibler, Camille N</name>
      </author>
      <author>
        <name>Cantalupo, Sebastiano</name>
      </author>
      <author>
        <name>Holden, Bradford P</name>
        <uri>https://orcid.org/0000-0002-6153-3076</uri>
      </author>
      <author>
        <name>Madau, Piero</name>
        <uri>https://orcid.org/0000-0002-6336-3293</uri>
      </author>
    </item>
    <item>
      <title>Iceline variations driven by protoplanetary disc gaps</title>
      <link>https://escholarship.org/uc/item/6h73h7jm</link>
      <description>ABSTRACT: 

               The composition of forming planets is strongly affected by the protoplanetary disc’s thermal structure. This thermal structure is predominantly set by dust radiative transfer and viscous (accretional) heating and can be impacted by gaps – regions of low dust and gas density that can occur when planets form. The effect of variations in dust surface density on disc temperature has been poorly understood to date. In this work, we use the radiative transfer code MCMax to model the 2D dust thermal structure with individual gaps corresponding to planets with masses of 0.1 MJ –5 MJ and orbital radii of 3, 5, and 10 au. Low dust opacity in the gap allows radiation to penetrate deeper and warm the mid-plane by up to 16&amp;nbsp;K, but only for gaps located in the region of the disc where stellar irradiation is the dominant source of heating. In viscously heated regions, the mid-plane of the gap is relatively cooler by up to 100&amp;nbsp;K. Outside of the gap, broad radial...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/6h73h7jm</guid>
      <pubDate>Thu, 14 Sep 2023 00:00:00 +0000</pubDate>
      <author>
        <name>Broome, Madelyn</name>
      </author>
      <author>
        <name>Kama, Mihkel</name>
      </author>
      <author>
        <name>Booth, Richard</name>
      </author>
      <author>
        <name>Shorttle, Oliver</name>
      </author>
    </item>
    <item>
      <title>Resolved imaging confirms a radiation belt around an ultracool dwarf</title>
      <link>https://escholarship.org/uc/item/0m5734s7</link>
      <description>Radiation belts are present in all large-scale Solar System planetary magnetospheres: Earth, Jupiter, Saturn, Uranus and Neptune1. These persistent equatorial zones of relativistic particles up to tens of megaelectron volts in energy can extend further than ten times the planet’s radius, emit gradually varying radio emissions2–4 and affect the surface chemistry of close-in moons5. Recent observations demonstrate that very low-mass stars and brown dwarfs, collectively known as ultracool dwarfs, can produce planet-like radio emissions such as periodically bursting aurorae6–8 from large-scale magnetospheric currents9–11. They also exhibit slowly varying quiescent radio emissions7,12,13 hypothesized to trace low-level coronal flaring14,15 despite departing from empirical multiwavelength flare relationships8,15. Here we present high-resolution imaging of the ultracool dwarf LSR J1835 + 3259 at 8.4 GHz, demonstrating that its quiescent radio emission is spatially resolved and traces...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/0m5734s7</guid>
      <pubDate>Sat, 2 Sep 2023 00:00:00 +0000</pubDate>
      <author>
        <name>Kao, Melodie M</name>
      </author>
      <author>
        <name>Mioduszewski, Amy J</name>
      </author>
      <author>
        <name>Villadsen, Jackie</name>
      </author>
      <author>
        <name>Shkolnik, Evgenya L</name>
      </author>
    </item>
    <item>
      <title>Identification of carbon dioxide in an exoplanet atmosphere</title>
      <link>https://escholarship.org/uc/item/25h1s5ms</link>
      <description>Carbon dioxide (CO2) is a key chemical species that is found in a wide range of planetary atmospheres. In the context of exoplanets, CO2 is an indicator of the metal enrichment (that is, elements heavier than helium, also called ‘metallicity’)1–3, and thus the formation processes of the primary atmospheres of hot gas giants4–6. It is also one of the most promising species to detect in the secondary atmospheres of terrestrial exoplanets7–9. Previous photometric measurements of transiting planets with the Spitzer Space Telescope have given hints of the presence of CO2, but have not yielded definitive detections owing to the lack of unambiguous spectroscopic identification10–12. Here we present the detection of CO2 in the atmosphere of the gas giant exoplanet WASP-39b from transmission spectroscopy observations obtained with&amp;nbsp;JWST as part of the Early Release Science programme13,14. The data used in this study span 3.0–5.5 micrometres in wavelength and show a prominent CO2 absorption...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/25h1s5ms</guid>
      <pubDate>Wed, 12 Jul 2023 00:00:00 +0000</pubDate>
      <author>
        <name>Ahrer, Eva-Maria</name>
      </author>
      <author>
        <name>Alderson, Lili</name>
      </author>
      <author>
        <name>Batalha, Natalie M</name>
      </author>
      <author>
        <name>Batalha, Natasha E</name>
      </author>
      <author>
        <name>Bean, Jacob L</name>
      </author>
      <author>
        <name>Beatty, Thomas G</name>
      </author>
      <author>
        <name>Bell, Taylor J</name>
      </author>
      <author>
        <name>Benneke, Björn</name>
      </author>
      <author>
        <name>Berta-Thompson, Zachory K</name>
      </author>
      <author>
        <name>Carter, Aarynn L</name>
      </author>
      <author>
        <name>Crossfield, Ian JM</name>
      </author>
      <author>
        <name>Espinoza, Néstor</name>
      </author>
      <author>
        <name>Feinstein, Adina D</name>
      </author>
      <author>
        <name>Fortney, Jonathan J</name>
      </author>
      <author>
        <name>Gibson, Neale P</name>
      </author>
      <author>
        <name>Goyal, Jayesh M</name>
      </author>
      <author>
        <name>Kempton, Eliza M-R</name>
      </author>
      <author>
        <name>Kirk, James</name>
      </author>
      <author>
        <name>Kreidberg, Laura</name>
      </author>
      <author>
        <name>López-Morales, Mercedes</name>
      </author>
      <author>
        <name>Line, Michael R</name>
      </author>
      <author>
        <name>Lothringer, Joshua D</name>
      </author>
      <author>
        <name>Moran, Sarah E</name>
      </author>
      <author>
        <name>Mukherjee, Sagnick</name>
      </author>
      <author>
        <name>Ohno, Kazumasa</name>
      </author>
      <author>
        <name>Parmentier, Vivien</name>
      </author>
      <author>
        <name>Piaulet, Caroline</name>
      </author>
      <author>
        <name>Rustamkulov, Zafar</name>
      </author>
      <author>
        <name>Schlawin, Everett</name>
      </author>
      <author>
        <name>Sing, David K</name>
      </author>
      <author>
        <name>Stevenson, Kevin B</name>
      </author>
      <author>
        <name>Wakeford, Hannah R</name>
      </author>
      <author>
        <name>Allen, Natalie H</name>
      </author>
      <author>
        <name>Birkmann, Stephan M</name>
      </author>
      <author>
        <name>Brande, Jonathan</name>
      </author>
      <author>
        <name>Crouzet, Nicolas</name>
      </author>
      <author>
        <name>Cubillos, Patricio E</name>
      </author>
      <author>
        <name>Damiano, Mario</name>
      </author>
      <author>
        <name>Désert, Jean-Michel</name>
      </author>
      <author>
        <name>Gao, Peter</name>
      </author>
      <author>
        <name>Harrington, Joseph</name>
      </author>
      <author>
        <name>Hu, Renyu</name>
      </author>
      <author>
        <name>Kendrew, Sarah</name>
      </author>
      <author>
        <name>Knutson, Heather A</name>
      </author>
      <author>
        <name>Lagage, Pierre-Olivier</name>
      </author>
      <author>
        <name>Leconte, Jérémy</name>
      </author>
      <author>
        <name>Lendl, Monika</name>
      </author>
      <author>
        <name>MacDonald, Ryan J</name>
      </author>
      <author>
        <name>May, EM</name>
      </author>
      <author>
        <name>Miguel, Yamila</name>
      </author>
      <author>
        <name>Molaverdikhani, Karan</name>
      </author>
      <author>
        <name>Moses, Julianne I</name>
      </author>
      <author>
        <name>Murray, Catriona Anne</name>
      </author>
      <author>
        <name>Nehring, Molly</name>
      </author>
      <author>
        <name>Nikolov, Nikolay K</name>
      </author>
      <author>
        <name>de la Roche, DJM Petit dit</name>
      </author>
      <author>
        <name>Radica, Michael</name>
      </author>
      <author>
        <name>Roy, Pierre-Alexis</name>
      </author>
      <author>
        <name>Stassun, Keivan G</name>
      </author>
      <author>
        <name>Taylor, Jake</name>
      </author>
      <author>
        <name>Waalkes, William C</name>
      </author>
      <author>
        <name>Wachiraphan, Patcharapol</name>
      </author>
      <author>
        <name>Welbanks, Luis</name>
      </author>
      <author>
        <name>Wheatley, Peter J</name>
      </author>
      <author>
        <name>Aggarwal, Keshav</name>
      </author>
      <author>
        <name>Alam, Munazza K</name>
      </author>
      <author>
        <name>Banerjee, Agnibha</name>
      </author>
      <author>
        <name>Barstow, Joanna K</name>
      </author>
      <author>
        <name>Blecic, Jasmina</name>
      </author>
      <author>
        <name>Casewell, SL</name>
      </author>
      <author>
        <name>Changeat, Quentin</name>
      </author>
      <author>
        <name>Chubb, KL</name>
      </author>
      <author>
        <name>Colón, Knicole D</name>
      </author>
      <author>
        <name>Coulombe, Louis-Philippe</name>
      </author>
      <author>
        <name>Daylan, Tansu</name>
      </author>
      <author>
        <name>de Val-Borro, Miguel</name>
      </author>
      <author>
        <name>Decin, Leen</name>
      </author>
      <author>
        <name>Dos Santos, Leonardo A</name>
      </author>
      <author>
        <name>Flagg, Laura</name>
      </author>
      <author>
        <name>France, Kevin</name>
      </author>
      <author>
        <name>Fu, Guangwei</name>
      </author>
      <author>
        <name>Muñoz, A García</name>
      </author>
      <author>
        <name>Gizis, John E</name>
      </author>
      <author>
        <name>Glidden, Ana</name>
      </author>
      <author>
        <name>Grant, David</name>
      </author>
      <author>
        <name>Heng, Kevin</name>
      </author>
      <author>
        <name>Henning, Thomas</name>
      </author>
      <author>
        <name>Hong, Yu-Cian</name>
      </author>
      <author>
        <name>Inglis, Julie</name>
      </author>
      <author>
        <name>Iro, Nicolas</name>
      </author>
      <author>
        <name>Kataria, Tiffany</name>
      </author>
      <author>
        <name>Komacek, Thaddeus D</name>
      </author>
      <author>
        <name>Krick, Jessica E</name>
      </author>
      <author>
        <name>Lee, Elspeth KH</name>
      </author>
      <author>
        <name>Lewis, Nikole K</name>
      </author>
      <author>
        <name>Lillo-Box, Jorge</name>
      </author>
      <author>
        <name>Lustig-Yaeger, Jacob</name>
      </author>
      <author>
        <name>Mancini, Luigi</name>
      </author>
      <author>
        <name>Mandell, Avi M</name>
      </author>
      <author>
        <name>Mansfield, Megan</name>
      </author>
    </item>
    <item>
      <title>Atmospheric characterization of terrestrial exoplanets in the mid-infrared: biosignatures, habitability, and diversity</title>
      <link>https://escholarship.org/uc/item/38h8p5qr</link>
      <description>Exoplanet science is one of the most thriving fields of modern astrophysics. A major goal is the atmospheric characterization of dozens of small, terrestrial exoplanets in order to search for signatures in their atmospheres that indicate biological activity, assess their ability to provide conditions for life as we know it, and investigate their expected atmospheric diversity. None of the currently adopted projects or missions, from ground or in space, can address these goals. In this White Paper, submitted to ESA in response to the Voyage 2050 Call, we argue that a large space-based mission designed to detect and investigate thermal emission spectra of terrestrial exoplanets in the mid-infrared wavelength range provides unique scientific potential to address these goals and surpasses the capabilities of other approaches. While NASA might be focusing on large missions that aim to detect terrestrial planets in reflected light, ESA has the opportunity to take leadership and spearhead...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/38h8p5qr</guid>
      <pubDate>Tue, 4 Jul 2023 00:00:00 +0000</pubDate>
      <author>
        <name>Quanz, Sascha P</name>
      </author>
      <author>
        <name>Absil, Olivier</name>
      </author>
      <author>
        <name>Benz, Willy</name>
      </author>
      <author>
        <name>Bonfils, Xavier</name>
      </author>
      <author>
        <name>Berger, Jean-Philippe</name>
      </author>
      <author>
        <name>Defrère, Denis</name>
      </author>
      <author>
        <name>van Dishoeck, Ewine</name>
      </author>
      <author>
        <name>Ehrenreich, David</name>
      </author>
      <author>
        <name>Fortney, Jonathan</name>
        <uri>https://orcid.org/0000-0002-9843-4354</uri>
      </author>
      <author>
        <name>Glauser, Adrian</name>
      </author>
      <author>
        <name>Grenfell, John Lee</name>
      </author>
      <author>
        <name>Janson, Markus</name>
      </author>
      <author>
        <name>Kraus, Stefan</name>
      </author>
      <author>
        <name>Krause, Oliver</name>
      </author>
      <author>
        <name>Labadie, Lucas</name>
      </author>
      <author>
        <name>Lacour, Sylvestre</name>
      </author>
      <author>
        <name>Line, Michael</name>
      </author>
      <author>
        <name>Linz, Hendrik</name>
      </author>
      <author>
        <name>Loicq, Jérôme</name>
      </author>
      <author>
        <name>Miguel, Yamila</name>
      </author>
      <author>
        <name>Pallé, Enric</name>
      </author>
      <author>
        <name>Queloz, Didier</name>
      </author>
      <author>
        <name>Rauer, Heike</name>
      </author>
      <author>
        <name>Ribas, Ignasi</name>
      </author>
      <author>
        <name>Rugheimer, Sarah</name>
      </author>
      <author>
        <name>Selsis, Franck</name>
      </author>
      <author>
        <name>Snellen, Ignas</name>
      </author>
      <author>
        <name>Sozzetti, Alessandro</name>
      </author>
      <author>
        <name>Stapelfeldt, Karl R</name>
      </author>
      <author>
        <name>Udry, Stephane</name>
      </author>
      <author>
        <name>Wyatt, Mark</name>
      </author>
    </item>
    <item>
      <title>COMPOSITIONAL DIVERSITY IN THE ATMOSPHERES OF HOT NEPTUNES, WITH APPLICATION TO GJ 436b</title>
      <link>https://escholarship.org/uc/item/51p7w7q2</link>
      <description>Neptune-sized extrasolar planets that orbit relatively close to their host stars - often called "hot Neptunes" - are common within the known population of exoplanets and planetary candidates. Similar to our own Uranus and Neptune, inefficient accretion of nebular gas is expected produce hot Neptunes whose masses are dominated by elements heavier than hydrogen and helium. At high atmospheric metallicities of 10-10,000× solar, hot Neptunes will exhibit an interesting continuum of atmospheric compositions, ranging from more Neptune-like, H&lt;sub&gt;2&lt;/sub&gt;-dominated atmospheres to more Venus-like, CO&lt;sub&gt;2&lt;/sub&gt;-dominated atmospheres. We explore the predicted equilibrium and disequilibrium chemistry of generic hot Neptunes and find that the atmospheric composition varies strongly as a function of temperature and bulk atmospheric properties such as metallicity and the C/O ratio. Relatively exotic H&lt;sub&gt;2&lt;/sub&gt;O, CO, CO&lt;sub&gt;2&lt;/sub&gt;, and even O&lt;sub&gt;2&lt;/sub&gt;-dominated atmospheres are possible...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/51p7w7q2</guid>
      <pubDate>Thu, 20 Apr 2023 00:00:00 +0000</pubDate>
      <author>
        <name>Moses, JI</name>
      </author>
      <author>
        <name>Line, MR</name>
      </author>
      <author>
        <name>Visscher, C</name>
      </author>
      <author>
        <name>Richardson, MR</name>
      </author>
      <author>
        <name>Nettelmann, N</name>
      </author>
      <author>
        <name>Fortney, JJ</name>
        <uri>https://orcid.org/0000-0002-9843-4354</uri>
      </author>
      <author>
        <name>Barman, TS</name>
      </author>
      <author>
        <name>Stevenson, KB</name>
      </author>
      <author>
        <name>Madhusudhan, N</name>
      </author>
    </item>
    <item>
      <title>Poisson_CCD: A dedicated simulator for modeling CCDs</title>
      <link>https://escholarship.org/uc/item/48v0b1g1</link>
      <description>A dedicated simulator, Poisson_CCD, has been constructed which models astronomical CCDs by solving Poisson’s equation numerically and simulating charge transport within the CCD. The potentials and free carrier densities within the CCD are self-consistently solved for, giving realistic results for the charge distribution within the CCD storage wells. The simulator has been used to model the CCDs that are being used to construct the LSST digital camera. The simulator output has been validated by comparing its predictions with several different types of CCD measurements, including astrometric shifts, brighter-fatter induced pixel–pixel covariances, saturation effects, and diffusion spreading. The code is open source and freely available.</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/48v0b1g1</guid>
      <pubDate>Mon, 10 Apr 2023 00:00:00 +0000</pubDate>
      <author>
        <name>Lage, Craig</name>
      </author>
      <author>
        <name>Bradshaw, Andrew</name>
        <uri>https://orcid.org/0000-0002-8998-6739</uri>
      </author>
      <author>
        <name>Tyson, J Anthony</name>
      </author>
    </item>
    <item>
      <title>Deep Exploration of ϵ Eridani with Keck Ms-band Vortex Coronagraphy and Radial Velocities: Mass and Orbital Parameters of the Giant Exoplanet* * Based on observations obtained at the W. M. Keck Observatory, which is operated jointly by the University of California and the California Institute of Technology. Keck time was granted for this project by Caltech, the University of Hawai’i, the University of California, and NASA.</title>
      <link>https://escholarship.org/uc/item/8bt1j548</link>
      <description>We present the most sensitive direct imaging and radial velocity (RV) exploration of Eridani to date. Eridani is an adolescent planetary system, reminiscent of the early solar system. It is surrounded by a prominent and complex debris disk that is likely stirred by one or several gas giant exoplanets. The discovery of the RV signature of a giant exoplanet was announced 15 yr ago, but has met with scrutiny due to possible confusion with stellar noise. We confirm the planet with a new compilation and analysis of precise RV data spanning 30 yr, and combine it with upper limits from our direct imaging search, the most sensitive ever performed. The deep images were taken in the Ms band (4.7 μm) with the vortex coronagraph recently installed in W.M. Keck Observatory's infrared camera NIRC2, which opens a sensitive window for planet searches around nearby adolescent systems. The RV data and direct imaging upper limit maps were combined in an innovative joint Bayesian analysis, providing...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/8bt1j548</guid>
      <pubDate>Thu, 5 Jan 2023 00:00:00 +0000</pubDate>
      <author>
        <name>Mawet, Dimitri</name>
      </author>
      <author>
        <name>Hirsch, Lea</name>
      </author>
      <author>
        <name>Lee, Eve J</name>
      </author>
      <author>
        <name>Ruffio, Jean-Baptiste</name>
      </author>
      <author>
        <name>Bottom, Michael</name>
      </author>
      <author>
        <name>Fulton, Benjamin J</name>
      </author>
      <author>
        <name>Absil, Olivier</name>
      </author>
      <author>
        <name>Beichman, Charles</name>
      </author>
      <author>
        <name>Bowler, Brendan</name>
      </author>
      <author>
        <name>Bryan, Marta</name>
      </author>
      <author>
        <name>Choquet, Elodie</name>
      </author>
      <author>
        <name>Ciardi, David</name>
      </author>
      <author>
        <name>Christiaens, Valentin</name>
      </author>
      <author>
        <name>Defrère, Denis</name>
      </author>
      <author>
        <name>Gonzalez, Carlos Alberto Gomez</name>
      </author>
      <author>
        <name>Howard, Andrew W</name>
      </author>
      <author>
        <name>Huby, Elsa</name>
      </author>
      <author>
        <name>Isaacson, Howard</name>
        <uri>https://orcid.org/0000-0002-0531-1073</uri>
      </author>
      <author>
        <name>Jensen-Clem, Rebecca</name>
        <uri>https://orcid.org/0000-0003-0054-2953</uri>
      </author>
      <author>
        <name>Kosiarek, Molly</name>
      </author>
      <author>
        <name>Marcy, Geoff</name>
        <uri>https://orcid.org/0000-0002-2909-0113</uri>
      </author>
      <author>
        <name>Meshkat, Tiffany</name>
      </author>
      <author>
        <name>Petigura, Erik</name>
      </author>
      <author>
        <name>Reggiani, Maddalena</name>
      </author>
      <author>
        <name>Ruane, Garreth</name>
      </author>
      <author>
        <name>Serabyn, Eugene</name>
      </author>
      <author>
        <name>Sinukoff, Evan</name>
      </author>
      <author>
        <name>Wang, Ji</name>
      </author>
      <author>
        <name>Weiss, Lauren</name>
      </author>
      <author>
        <name>Ygouf, Marie</name>
      </author>
    </item>
    <item>
      <title>The TESS–Keck Survey. I. A Warm Sub-Saturn-mass Planet and a Caution about Stray Light in TESS Cameras* * Some of the data presented herein were obtained at the W. M. Keck Observatory, which is operated as a scientific partnership among the California Institute of Technology, the University of California and the National Aeronautics and Space Administration. The Observatory was made possible by the generous financial support of the W. M. Keck Foundation.</title>
      <link>https://escholarship.org/uc/item/6t886683</link>
      <description>We report the detection of a Saturn-size exoplanet orbiting HD 332231 (TOI 1456) in light curves from the Transiting Exoplanet Survey Satellite (TESS). HD 332231 - an F8 dwarf star with a V-band magnitude of 8.56 - was observed by TESS in Sectors 14 and 15. We detect a single-transit event in the Sector 15 presearch data conditioning (PDC) light curve. We obtain spectroscopic follow-up observations of HD 332231 with the Automated Planet Finder, Keck I, and SONG telescopes. The orbital period we infer from radial velocity (RV) observations leads to the discovery of another transit in Sector 14 that was masked by PDC due to scattered light contamination. A joint analysis of the transit and RV data confirms the planetary nature of HD 332231 b, a Saturn-size (0.867-0.025+0.027RJ), sub-Saturn-mass (0.244±0.021MJ) exoplanet on a 18.71 day circular orbit. The low surface gravity of HD 332231 b and the relatively low stellar flux it receives make it a compelling target for transmission...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/6t886683</guid>
      <pubDate>Thu, 5 Jan 2023 00:00:00 +0000</pubDate>
      <author>
        <name>Dalba, Paul A</name>
      </author>
      <author>
        <name>Gupta, Arvind F</name>
      </author>
      <author>
        <name>Rodriguez, Joseph E</name>
      </author>
      <author>
        <name>Dragomir, Diana</name>
      </author>
      <author>
        <name>Huang, Chelsea X</name>
      </author>
      <author>
        <name>Kane, Stephen R</name>
        <uri>https://orcid.org/0000-0002-7084-0529</uri>
      </author>
      <author>
        <name>Quinn, Samuel N</name>
      </author>
      <author>
        <name>Bieryla, Allyson</name>
      </author>
      <author>
        <name>Esquerdo, Gilbert A</name>
      </author>
      <author>
        <name>Fulton, Benjamin J</name>
      </author>
      <author>
        <name>Scarsdale, Nicholas</name>
      </author>
      <author>
        <name>Batalha, Natalie M</name>
      </author>
      <author>
        <name>Beard, Corey</name>
      </author>
      <author>
        <name>Behmard, Aida</name>
      </author>
      <author>
        <name>Chontos, Ashley</name>
      </author>
      <author>
        <name>Crossfield, Ian JM</name>
      </author>
      <author>
        <name>Dressing, Courtney D</name>
        <uri>https://orcid.org/0000-0001-8189-0233</uri>
      </author>
      <author>
        <name>Giacalone, Steven</name>
      </author>
      <author>
        <name>Hill, Michelle L</name>
      </author>
      <author>
        <name>Hirsch, Lea A</name>
      </author>
      <author>
        <name>Howard, Andrew W</name>
      </author>
      <author>
        <name>Huber, Daniel</name>
      </author>
      <author>
        <name>Isaacson, Howard</name>
        <uri>https://orcid.org/0000-0002-0531-1073</uri>
      </author>
      <author>
        <name>Kosiarek, Molly</name>
      </author>
      <author>
        <name>Lubin, Jack</name>
      </author>
      <author>
        <name>Mayo, Andrew W</name>
      </author>
      <author>
        <name>Mocnik, Teo</name>
      </author>
      <author>
        <name>Murphy, Joseph M Akana</name>
      </author>
      <author>
        <name>Petigura, Erik A</name>
      </author>
      <author>
        <name>Robertson, Paul</name>
      </author>
      <author>
        <name>Rosenthal, Lee J</name>
      </author>
      <author>
        <name>Roy, Arpita</name>
      </author>
      <author>
        <name>Rubenzahl, Ryan A</name>
      </author>
      <author>
        <name>Van Zandt, Judah</name>
      </author>
      <author>
        <name>Weiss, Lauren M</name>
      </author>
      <author>
        <name>Knudstrup, Emil</name>
      </author>
      <author>
        <name>Andersen, Mads F</name>
      </author>
      <author>
        <name>Grundahl, Frank</name>
      </author>
      <author>
        <name>Yao, Xinyu</name>
      </author>
      <author>
        <name>Pepper, Joshua</name>
      </author>
      <author>
        <name>Villanueva, Steven</name>
      </author>
      <author>
        <name>Ciardi, David R</name>
      </author>
      <author>
        <name>Cloutier, Ryan</name>
      </author>
      <author>
        <name>Jacobs, Thomas Lee</name>
      </author>
      <author>
        <name>Kristiansen, Martti H</name>
      </author>
      <author>
        <name>LaCourse, Daryll M</name>
      </author>
      <author>
        <name>Lendl, Monika</name>
      </author>
      <author>
        <name>Osborn, Hugh P</name>
      </author>
      <author>
        <name>Palle, Enric</name>
      </author>
      <author>
        <name>Stassun, Keivan G</name>
      </author>
      <author>
        <name>Stevens, Daniel J</name>
      </author>
      <author>
        <name>Ricker, George R</name>
      </author>
      <author>
        <name>Vanderspek, Roland</name>
      </author>
      <author>
        <name>Latham, David W</name>
      </author>
      <author>
        <name>Seager, S</name>
      </author>
      <author>
        <name>Winn, Joshua N</name>
      </author>
      <author>
        <name>Jenkins, Jon M</name>
      </author>
      <author>
        <name>Caldwell, Douglas A</name>
      </author>
      <author>
        <name>Daylan, Tansu</name>
      </author>
      <author>
        <name>Fong, William</name>
      </author>
      <author>
        <name>Goeke, Robert F</name>
      </author>
      <author>
        <name>Rose, Mark E</name>
      </author>
      <author>
        <name>Rowden, Pamela</name>
      </author>
      <author>
        <name>Schlieder, Joshua E</name>
      </author>
      <author>
        <name>Smith, Jeffrey C</name>
      </author>
      <author>
        <name>Vanderburg, Andrew</name>
      </author>
    </item>
    <item>
      <title>The TESS-Keck Survey. III. A Stellar Obliquity Measurement of TOI-1726 c</title>
      <link>https://escholarship.org/uc/item/60f543qx</link>
      <description>We report the measurement of a spectroscopic transit of TOI-1726c, one of two planets transiting a G-type star with V = 6.9 in the Ursa Major Moving Group (∼400 Myr). With a precise age constraint from cluster membership, TOI-1726 provides a great opportunity to test various obliquity excitation scenarios that operate on different timescales. By modeling the Rossiter-McLaughlin (RM) effect, we derived a sky-projected obliquity of -1-+3235∘. This result rules out a polar/retrograde orbit and is consistent with an aligned orbit for planet c. Considering the previously reported, similarly prograde RM measurement of planet b and the transiting nature of both planets, TOI-1726 tentatively conforms to the overall picture that compact multitransiting planetary systems tend to have coplanar, likely aligned orbits. TOI-1726 is also a great atmospheric target for understanding differential atmospheric loss of sub-Neptune planets (planet b 2.2 R☉ and c 2.7 R☉ both likely underwent photoevaporation)....</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/60f543qx</guid>
      <pubDate>Thu, 5 Jan 2023 00:00:00 +0000</pubDate>
      <author>
        <name>Dai, Fei</name>
      </author>
      <author>
        <name>Roy, Arpita</name>
      </author>
      <author>
        <name>Fulton, Benjamin</name>
      </author>
      <author>
        <name>Robertson, Paul</name>
      </author>
      <author>
        <name>Hirsch, Lea</name>
      </author>
      <author>
        <name>Isaacson, Howard</name>
        <uri>https://orcid.org/0000-0002-0531-1073</uri>
      </author>
      <author>
        <name>Albrecht, Simon</name>
      </author>
      <author>
        <name>Mann, Andrew W</name>
      </author>
      <author>
        <name>Kristiansen, Martti H</name>
      </author>
      <author>
        <name>Batalha, Natalie M</name>
      </author>
      <author>
        <name>Beard, Corey</name>
      </author>
      <author>
        <name>Behmard, Aida</name>
      </author>
      <author>
        <name>Chontos, Ashley</name>
      </author>
      <author>
        <name>Crossfield, Ian JM</name>
      </author>
      <author>
        <name>Dalba, Paul A</name>
      </author>
      <author>
        <name>Dressing, Courtney</name>
        <uri>https://orcid.org/0000-0001-8189-0233</uri>
      </author>
      <author>
        <name>Giacalone, Steven</name>
      </author>
      <author>
        <name>Hill, Michelle</name>
      </author>
      <author>
        <name>Howard, Andrew W</name>
      </author>
      <author>
        <name>Huber, Daniel</name>
      </author>
      <author>
        <name>Kane, Stephen R</name>
        <uri>https://orcid.org/0000-0002-7084-0529</uri>
      </author>
      <author>
        <name>Kosiarek, Molly</name>
      </author>
      <author>
        <name>Lubin, Jack</name>
      </author>
      <author>
        <name>Mayo, Andrew</name>
      </author>
      <author>
        <name>Mocnik, Teo</name>
      </author>
      <author>
        <name>Murphy, Joseph M Akana</name>
      </author>
      <author>
        <name>Petigura, Erik A</name>
      </author>
      <author>
        <name>Rosenthal, Lee</name>
      </author>
      <author>
        <name>Rubenzahl, Ryan A</name>
      </author>
      <author>
        <name>Scarsdale, Nicholas</name>
      </author>
      <author>
        <name>Weiss, Lauren M</name>
      </author>
      <author>
        <name>Van Zandt, Judah</name>
      </author>
      <author>
        <name>Ricker, George R</name>
      </author>
      <author>
        <name>Vanderspek, Roland</name>
      </author>
      <author>
        <name>Latham, David W</name>
      </author>
      <author>
        <name>Seager, Sara</name>
      </author>
      <author>
        <name>Winn, Joshua N</name>
      </author>
      <author>
        <name>Jenkins, Jon M</name>
      </author>
      <author>
        <name>Caldwell, Douglas A</name>
      </author>
      <author>
        <name>Charbonneau, David</name>
      </author>
      <author>
        <name>Daylan, Tansu</name>
      </author>
      <author>
        <name>Günther, Maximilian N</name>
      </author>
      <author>
        <name>Morgan, Edward</name>
      </author>
      <author>
        <name>Quinn, Samuel N</name>
      </author>
      <author>
        <name>Rose, Mark E</name>
      </author>
      <author>
        <name>Smith, Jeffrey C</name>
      </author>
    </item>
    <item>
      <title>The TESS-Keck Survey. II. An Ultra-short-period Rocky Planet and Its Siblings Transiting the Galactic Thick-disk Star TOI-561</title>
      <link>https://escholarship.org/uc/item/5hj1h0bf</link>
      <description>We report the discovery of TOI-561, a multiplanet system in the galactic thick disk that contains a rocky, ultrashort- period planet. This bright (V = 10.2) star hosts three small transiting planets identified in photometry from the NASA TESS mission: TOI-561 b (TOI-561.02, P = 0.44 days, Rp = 1.45 ± 0.11 R⊕), c (TOI-561.01, P = 10.8 days, Rp = 2.90 ± 0.13 R⊕), and d (TOI-561.03, P = 16.3 days, Rp = 2.32 ± 0.16 R⊕). The star is chemically ([Fe/ H] = -0.41 ± 0.05, [a/Fe]=+0.23 ± 0.05) and kinematically consistent with the galactic thick-disk population, making TOI-561 one of the oldest (10 ± 3 Gyr) and most metal-poor planetary systems discovered yet. We dynamically confirm planets b and c with radial velocities from the W. M. Keck Observatory High Resolution Echelle Spectrometer. Planet b has a mass and density of 3.2 ± 0.8M⊕ and 5.5+2.0-1.6g cm-3, consistent with a rocky composition. Its lower-than-average density is consistent with an iron-poor composition, although an Earth-like...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/5hj1h0bf</guid>
      <pubDate>Thu, 5 Jan 2023 00:00:00 +0000</pubDate>
      <author>
        <name>Weiss, Lauren M</name>
      </author>
      <author>
        <name>Dai, Fei</name>
      </author>
      <author>
        <name>Huber, Daniel</name>
      </author>
      <author>
        <name>Brewer, John M</name>
      </author>
      <author>
        <name>Collins, Karen A</name>
      </author>
      <author>
        <name>Ciardi, David R</name>
      </author>
      <author>
        <name>Matthews, Elisabeth C</name>
      </author>
      <author>
        <name>Ziegler, Carl</name>
      </author>
      <author>
        <name>Howell, Steve B</name>
      </author>
      <author>
        <name>Batalha, Natalie M</name>
      </author>
      <author>
        <name>Crossfield, Ian JM</name>
      </author>
      <author>
        <name>Dressing, Courtney</name>
        <uri>https://orcid.org/0000-0001-8189-0233</uri>
      </author>
      <author>
        <name>Fulton, Benjamin</name>
      </author>
      <author>
        <name>Howard, Andrew W</name>
      </author>
      <author>
        <name>Isaacson, Howard</name>
        <uri>https://orcid.org/0000-0002-0531-1073</uri>
      </author>
      <author>
        <name>Kane, Stephen R</name>
        <uri>https://orcid.org/0000-0002-7084-0529</uri>
      </author>
      <author>
        <name>Petigura, Erik A</name>
      </author>
      <author>
        <name>Robertson, Paul</name>
      </author>
      <author>
        <name>Roy, Arpita</name>
      </author>
      <author>
        <name>Rubenzahl, Ryan A</name>
      </author>
      <author>
        <name>Twicken, Joseph D</name>
      </author>
      <author>
        <name>Claytor, Zachary R</name>
      </author>
      <author>
        <name>Stassun, Keivan G</name>
      </author>
      <author>
        <name>MacDougall, Mason G</name>
      </author>
      <author>
        <name>Chontos, Ashley</name>
      </author>
      <author>
        <name>Giacalone, Steven</name>
      </author>
      <author>
        <name>Dalba, Paul A</name>
      </author>
      <author>
        <name>Mocnik, Teo</name>
      </author>
      <author>
        <name>Hill, Michelle L</name>
      </author>
      <author>
        <name>Beard, Corey</name>
      </author>
      <author>
        <name>Murphy, Joseph M Akana</name>
      </author>
      <author>
        <name>Rosenthal, Lee J</name>
      </author>
      <author>
        <name>Behmard, Aida</name>
      </author>
      <author>
        <name>Van Zandt, Judah</name>
      </author>
      <author>
        <name>Lubin, Jack</name>
      </author>
      <author>
        <name>Kosiarek, Molly R</name>
      </author>
      <author>
        <name>Lund, Michael B</name>
      </author>
      <author>
        <name>Christiansen, Jessie L</name>
      </author>
      <author>
        <name>Matson, Rachel A</name>
      </author>
      <author>
        <name>Beichman, Charles A</name>
      </author>
      <author>
        <name>Schlieder, Joshua E</name>
      </author>
      <author>
        <name>Gonzales, Erica J</name>
      </author>
      <author>
        <name>Briceño, César</name>
      </author>
      <author>
        <name>Law, Nicholas</name>
      </author>
      <author>
        <name>Mann, Andrew W</name>
      </author>
      <author>
        <name>Collins, Kevin I</name>
      </author>
      <author>
        <name>Evans, Phil</name>
      </author>
      <author>
        <name>Fukui, Akihiko</name>
      </author>
      <author>
        <name>Jensen, Eric LN</name>
      </author>
      <author>
        <name>Murgas, Felipe</name>
      </author>
      <author>
        <name>Narita, Norio</name>
      </author>
      <author>
        <name>Palle, Enric</name>
      </author>
      <author>
        <name>Parviainen, Hannu</name>
      </author>
      <author>
        <name>Schwarz, Richard P</name>
      </author>
      <author>
        <name>Tan, Thiam-Guan</name>
      </author>
      <author>
        <name>Acton, Jack S</name>
      </author>
      <author>
        <name>Bryant, Edward M</name>
      </author>
      <author>
        <name>Chaushev, Alexander</name>
      </author>
      <author>
        <name>Gill, Sam</name>
      </author>
      <author>
        <name>Eigmüller, Philipp</name>
      </author>
      <author>
        <name>Jenkins, Jon</name>
      </author>
      <author>
        <name>Ricker, George</name>
      </author>
      <author>
        <name>Seager, Sara</name>
      </author>
      <author>
        <name>Winn, Joshua N</name>
      </author>
    </item>
    <item>
      <title>Updated Parameters and a New Transmission Spectrum of HD 97658b</title>
      <link>https://escholarship.org/uc/item/46v9r6jg</link>
      <description>Recent years have seen increasing interest in the characterization of sub-Neptune-sized planets because of their prevalence in the Galaxy, contrasted with their absence in our solar system. HD 97658 is one of the brightest stars hosting a planet of this kind, and we present the transmission spectrum of this planet by combining four Hubble Space Telescope transits, 12 Spitzer/IRAC transits, and eight MOST transits of this system. Our transmission spectrum has a higher signal-to-noise ratio than those from previous works, and the result suggests that the slight increase in transit depth from wavelength 1.1-1.7 μm reported in previous works on the transmission spectrum of this planet is likely systematic. Nonetheless, our atmospheric modeling results are inconclusive, as no model provides an excellent match to our data. Nonetheless, we find that atmospheres with high C/O ratios (C/O ≈ 0.8) and metallicities of ≈100× solar metallicity are favored. We combine the mid-transit times...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/46v9r6jg</guid>
      <pubDate>Thu, 5 Jan 2023 00:00:00 +0000</pubDate>
      <author>
        <name>Guo, Xueying</name>
      </author>
      <author>
        <name>Crossfield, Ian JM</name>
      </author>
      <author>
        <name>Dragomir, Diana</name>
      </author>
      <author>
        <name>Kosiarek, Molly R</name>
      </author>
      <author>
        <name>Lothringer, Joshua</name>
      </author>
      <author>
        <name>Mikal-Evans, Thomas</name>
      </author>
      <author>
        <name>Rosenthal, Lee</name>
      </author>
      <author>
        <name>Benneke, Bjorn</name>
      </author>
      <author>
        <name>Knutson, Heather A</name>
      </author>
      <author>
        <name>Dalba, Paul A</name>
      </author>
      <author>
        <name>Kempton, Eliza MR</name>
      </author>
      <author>
        <name>Henry, Gregory W</name>
      </author>
      <author>
        <name>McCullough, PR</name>
      </author>
      <author>
        <name>Barman, Travis</name>
      </author>
      <author>
        <name>Blunt, Sarah</name>
      </author>
      <author>
        <name>Chontos, Ashley</name>
      </author>
      <author>
        <name>Fortney, Jonathan</name>
        <uri>https://orcid.org/0000-0002-9843-4354</uri>
      </author>
      <author>
        <name>Fulton, Benjamin J</name>
      </author>
      <author>
        <name>Hirsch, Lea</name>
      </author>
      <author>
        <name>Howard, Andrew W</name>
      </author>
      <author>
        <name>Isaacson, Howard</name>
        <uri>https://orcid.org/0000-0002-0531-1073</uri>
      </author>
      <author>
        <name>Matthews, Jaymie</name>
      </author>
      <author>
        <name>Mocnik, Teo</name>
      </author>
      <author>
        <name>Morley, Caroline</name>
      </author>
      <author>
        <name>Petigura, Erik A</name>
      </author>
      <author>
        <name>Weiss, Lauren M</name>
      </author>
    </item>
    <item>
      <title>TOI-1235 b: A Keystone Super-Earth for Testing Radius Valley Emergence Models around Early M Dwarfs</title>
      <link>https://escholarship.org/uc/item/4285d4s1</link>
      <description>Small planets on close-in orbits tend to exhibit envelope mass fractions of either effectively zero or up to a few percent depending on their size and orbital period. Models of thermally driven atmospheric mass loss and of terrestrial planet formation in a gas-poor environment make distinct predictions regarding the location of this rocky/nonrocky transition in period-radius space. Here we present the confirmation of TOI-1235 b (P = 3.44 days, rp1.738-0.076+0.087 R⊕), a planet whose size and period are intermediate between the competing model predictions, thus making the system an important test case for emergence models of the rocky/nonrocky transition around early M dwarfs (R s = 0.630± 0.015 ⊕, M s = 0.640 ± 0.016 ⊙. We confirm the TESS planet discovery using reconnaissance spectroscopy, ground-based photometry, high-resolution imaging, and a set of 38 precise radial velocities (RVs) from HARPS-N and HIRES. We measure a planet mass of 6.91-0.85+0.75M⊕ which implies an iron...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/4285d4s1</guid>
      <pubDate>Thu, 5 Jan 2023 00:00:00 +0000</pubDate>
      <author>
        <name>Cloutier, Ryan</name>
      </author>
      <author>
        <name>Rodriguez, Joseph E</name>
      </author>
      <author>
        <name>Irwin, Jonathan</name>
      </author>
      <author>
        <name>Charbonneau, David</name>
      </author>
      <author>
        <name>Stassun, Keivan G</name>
      </author>
      <author>
        <name>Mortier, Annelies</name>
      </author>
      <author>
        <name>Latham, David W</name>
      </author>
      <author>
        <name>Isaacson, Howard</name>
        <uri>https://orcid.org/0000-0002-0531-1073</uri>
      </author>
      <author>
        <name>Howard, Andrew W</name>
      </author>
      <author>
        <name>Udry, Stéphane</name>
      </author>
      <author>
        <name>Wilson, Thomas G</name>
      </author>
      <author>
        <name>Watson, Christopher A</name>
      </author>
      <author>
        <name>Pinamonti, Matteo</name>
      </author>
      <author>
        <name>Lienhard, Florian</name>
      </author>
      <author>
        <name>Giacobbe, Paolo</name>
      </author>
      <author>
        <name>Guerra, Pere</name>
      </author>
      <author>
        <name>Collins, Karen A</name>
      </author>
      <author>
        <name>Beiryla, Allyson</name>
      </author>
      <author>
        <name>Esquerdo, Gilbert A</name>
      </author>
      <author>
        <name>Matthews, Elisabeth</name>
      </author>
      <author>
        <name>Matson, Rachel A</name>
      </author>
      <author>
        <name>Howell, Steve B</name>
      </author>
      <author>
        <name>Furlan, Elise</name>
      </author>
      <author>
        <name>Crossfield, Ian JM</name>
      </author>
      <author>
        <name>Winters, Jennifer G</name>
      </author>
      <author>
        <name>Nava, Chantanelle</name>
      </author>
      <author>
        <name>Ment, Kristo</name>
      </author>
      <author>
        <name>Lopez, Eric D</name>
      </author>
      <author>
        <name>Ricker, George</name>
      </author>
      <author>
        <name>Vanderspek, Roland</name>
      </author>
      <author>
        <name>Seager, Sara</name>
      </author>
      <author>
        <name>Jenkins, Jon M</name>
      </author>
      <author>
        <name>Ting, Eric B</name>
      </author>
      <author>
        <name>Tenenbaum, Peter</name>
      </author>
      <author>
        <name>Sozzetti, Alessandro</name>
      </author>
      <author>
        <name>Sha, Lizhou</name>
      </author>
      <author>
        <name>Ségransan, Damien</name>
      </author>
      <author>
        <name>Schlieder, Joshua E</name>
      </author>
      <author>
        <name>Sasselov, Dimitar</name>
      </author>
      <author>
        <name>Roy, Arpita</name>
      </author>
      <author>
        <name>Robertson, Paul</name>
      </author>
      <author>
        <name>Rice, Ken</name>
      </author>
      <author>
        <name>Poretti, Ennio</name>
      </author>
      <author>
        <name>Piotto, Giampaolo</name>
      </author>
      <author>
        <name>Phillips, David</name>
      </author>
      <author>
        <name>Pepper, Joshua</name>
      </author>
      <author>
        <name>Pepe, Francesco</name>
      </author>
      <author>
        <name>Molinari, Emilio</name>
      </author>
      <author>
        <name>Mocnik, Teo</name>
      </author>
      <author>
        <name>Micela, Giuseppina</name>
      </author>
      <author>
        <name>Mayor, Michel</name>
      </author>
      <author>
        <name>Fiorenzano, Aldo F Martinez</name>
      </author>
      <author>
        <name>Mallia, Franco</name>
      </author>
      <author>
        <name>Lubin, Jack</name>
      </author>
      <author>
        <name>Lovis, Christophe</name>
      </author>
      <author>
        <name>López-Morales, Mercedes</name>
      </author>
      <author>
        <name>Kosiarek, Molly R</name>
      </author>
      <author>
        <name>Kielkopf, John F</name>
      </author>
      <author>
        <name>Kane, Stephen R</name>
        <uri>https://orcid.org/0000-0002-7084-0529</uri>
      </author>
      <author>
        <name>Jensen, Eric LN</name>
      </author>
      <author>
        <name>Isopi, Giovanni</name>
      </author>
      <author>
        <name>Huber, Daniel</name>
      </author>
      <author>
        <name>Hill, Michelle L</name>
      </author>
      <author>
        <name>Harutyunyan, Avet</name>
      </author>
      <author>
        <name>Gonzales, Erica</name>
      </author>
      <author>
        <name>Giacalone, Steven</name>
      </author>
      <author>
        <name>Ghedina, Adriano</name>
      </author>
      <author>
        <name>Ercolino, Andrea</name>
      </author>
      <author>
        <name>Dumusque, Xavier</name>
      </author>
      <author>
        <name>Dressing, Courtney D</name>
        <uri>https://orcid.org/0000-0001-8189-0233</uri>
      </author>
      <author>
        <name>Damasso, Mario</name>
      </author>
      <author>
        <name>Dalba, Paul A</name>
      </author>
      <author>
        <name>Cosentino, Rosario</name>
      </author>
      <author>
        <name>Conti, Dennis M</name>
      </author>
      <author>
        <name>Colón, Knicole D</name>
      </author>
      <author>
        <name>Collins, Kevin I</name>
      </author>
      <author>
        <name>Cameron, Andrew Collier</name>
      </author>
      <author>
        <name>Ciardi, David</name>
      </author>
      <author>
        <name>Christiansen, Jessie</name>
      </author>
      <author>
        <name>Chontos, Ashley</name>
      </author>
      <author>
        <name>Cecconi, Massimo</name>
      </author>
      <author>
        <name>Caldwell, Douglas A</name>
      </author>
      <author>
        <name>Burke, Christopher</name>
      </author>
      <author>
        <name>Buchhave, Lars</name>
      </author>
      <author>
        <name>Beichman, Charles</name>
      </author>
      <author>
        <name>Behmard, Aida</name>
      </author>
      <author>
        <name>Beard, Corey</name>
      </author>
      <author>
        <name>Murphy, Joseph M Akana</name>
      </author>
    </item>
    <item>
      <title>Physical Parameters of the Multiplanet Systems HD 106315 and GJ 9827* *Based on observations obtained at the W. M. Keck Observatory, which is operated jointly by the University of California and the California Institute of Technology. † †This paper includes data gathered with the 6.5 meter Magellan Telescopes located at Las Campanas Observatory, Chile.</title>
      <link>https://escholarship.org/uc/item/3zj9d3xg</link>
      <description>HD 106315 and GJ 9827 are two bright, nearby stars that host multiple super-Earths and sub-Neptunes discovered by K2 that are well suited for atmospheric characterization. We refined the planets' ephemerides through Spitzer transits, enabling accurate transit prediction required for future atmospheric characterization through transmission spectroscopy. Through a multiyear high-cadence observing campaign with Keck/High Resolution Echelle Spectrometer and Magellan/Planet Finder Spectrograph, we improved the planets' mass measurements in anticipation of Hubble Space Telescope transmission spectroscopy. For GJ 9827, we modeled activity-induced radial velocity signals with a Gaussian process informed by the Calcium II H&amp;amp;K lines in order to more accurately model the effect of stellar noise on our data. We measured planet masses of Mb = 4.87 ± 0.37 M⊕, Mc = 1.92 ± 0.49 M⊕, and Md = 3.42 ± 0.62 M⊕. For HD 106315, we found that such activity radial velocity decorrelation was not effective...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/3zj9d3xg</guid>
      <pubDate>Thu, 5 Jan 2023 00:00:00 +0000</pubDate>
      <author>
        <name>Kosiarek, Molly R</name>
      </author>
      <author>
        <name>Berardo, David A</name>
      </author>
      <author>
        <name>Crossfield, Ian JM</name>
      </author>
      <author>
        <name>Laguna, Cesar</name>
      </author>
      <author>
        <name>Piaulet, Caroline</name>
      </author>
      <author>
        <name>Murphy, Joseph M Akana</name>
      </author>
      <author>
        <name>Howell, Steve B</name>
      </author>
      <author>
        <name>Henry, Gregory W</name>
      </author>
      <author>
        <name>Isaacson, Howard</name>
        <uri>https://orcid.org/0000-0002-0531-1073</uri>
      </author>
      <author>
        <name>Fulton, Benjamin</name>
      </author>
      <author>
        <name>Weiss, Lauren M</name>
      </author>
      <author>
        <name>Petigura, Erik A</name>
      </author>
      <author>
        <name>Behmard, Aida</name>
      </author>
      <author>
        <name>Hirsch, Lea A</name>
      </author>
      <author>
        <name>Teske, Johanna</name>
      </author>
      <author>
        <name>Burt, Jennifer A</name>
      </author>
      <author>
        <name>Mills, Sean M</name>
      </author>
      <author>
        <name>Chontos, Ashley</name>
      </author>
      <author>
        <name>Močnik, Teo</name>
      </author>
      <author>
        <name>Howard, Andrew W</name>
      </author>
      <author>
        <name>Werner, Michael</name>
      </author>
      <author>
        <name>Livingston, John H</name>
      </author>
      <author>
        <name>Krick, Jessica</name>
      </author>
      <author>
        <name>Beichman, Charles</name>
      </author>
      <author>
        <name>Gorjian, Varoujan</name>
      </author>
      <author>
        <name>Kreidberg, Laura</name>
      </author>
      <author>
        <name>Morley, Caroline</name>
      </author>
      <author>
        <name>Christiansen, Jessie L</name>
      </author>
      <author>
        <name>Morales, Farisa Y</name>
      </author>
      <author>
        <name>Scott, Nicholas J</name>
      </author>
      <author>
        <name>Crane, Jeffrey D</name>
      </author>
      <author>
        <name>Wang, Sharon Xuesong</name>
      </author>
      <author>
        <name>Shectman, Stephen A</name>
      </author>
      <author>
        <name>Rosenthal, Lee J</name>
      </author>
      <author>
        <name>Grunblatt, Samuel K</name>
      </author>
      <author>
        <name>Rubenzahl, Ryan A</name>
      </author>
      <author>
        <name>Dalba, Paul A</name>
      </author>
      <author>
        <name>Giacalone, Steven</name>
      </author>
      <author>
        <name>Villanueva, Chiara Dane</name>
      </author>
      <author>
        <name>Liu, Qingtian</name>
      </author>
      <author>
        <name>Dai, Fei</name>
      </author>
      <author>
        <name>Hill, Michelle L</name>
      </author>
      <author>
        <name>Rice, Malena</name>
      </author>
      <author>
        <name>Kane, Stephen R</name>
        <uri>https://orcid.org/0000-0002-7084-0529</uri>
      </author>
      <author>
        <name>Mayo, Andrew W</name>
      </author>
    </item>
    <item>
      <title>Validation and Initial Characterization of the Long-period Planet Kepler-1654 b</title>
      <link>https://escholarship.org/uc/item/3gc963s0</link>
      <description>Fewer than 20 transiting Kepler planets have periods longer than one year. Our early search of the Kepler light curves revealed one such system, Kepler-1654b (originally KIC 8410697b), which shows exactly two transit events and whose second transit occurred only five days before the failure of the second of two reaction wheels brought the primary Kepler mission to an end. A number of authors have also examined light curves from the Kepler mission searching for long-period planets and identified this candidate. Starting in 2014 September, we began an observational program of imaging, reconnaissance spectroscopy, and precision radial velocity (RV) measurements that confirm with a high degree of confidence that Kepler-1654b is a bona fide transiting planet orbiting a mature G5V star (T eff = 5580 K, [Fe/H] = -0.08) with a semimajor axis of 2.03 au, a period of 1047.84 days, and a radius of 0.82 ±0.02 R Jup. RV measurements using Keck's HIRES spectrometer obtained over 2.5 years set...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/3gc963s0</guid>
      <pubDate>Thu, 5 Jan 2023 00:00:00 +0000</pubDate>
      <author>
        <name>Beichman, CA</name>
      </author>
      <author>
        <name>Giles, HAC</name>
      </author>
      <author>
        <name>Akeson, R</name>
      </author>
      <author>
        <name>Ciardi, D</name>
      </author>
      <author>
        <name>Christiansen, J</name>
      </author>
      <author>
        <name>Isaacson, H</name>
        <uri>https://orcid.org/0000-0002-0531-1073</uri>
      </author>
      <author>
        <name>Marcy, GM</name>
        <uri>https://orcid.org/0000-0002-2909-0113</uri>
      </author>
      <author>
        <name>Sinukoff, E</name>
      </author>
      <author>
        <name>Greene, T</name>
      </author>
      <author>
        <name>Fortney, JJ</name>
        <uri>https://orcid.org/0000-0002-9843-4354</uri>
      </author>
      <author>
        <name>Crossfield, I</name>
      </author>
      <author>
        <name>Hu, R</name>
      </author>
      <author>
        <name>Howard, AW</name>
      </author>
      <author>
        <name>Petigura, EA</name>
      </author>
      <author>
        <name>Knutson, HA</name>
      </author>
    </item>
    <item>
      <title>The TESS–Keck Survey. IV. A Retrograde, Polar Orbit for the Ultra-low-density, Hot Super-Neptune WASP-107b</title>
      <link>https://escholarship.org/uc/item/39c8w4h4</link>
      <description>We measured the Rossiter-McLaughlin effect of WASP-107b during a single transit with Keck/HIRES. We found the sky-projected inclination of WASP-107b's orbit, relative to its host star's rotation axis, to be |λ| = 118+19-38degrees. This confirms the misaligned/polar orbit that was previously suggested from spot-crossing events and adds WASP-107b to the growing population of hot Neptunes in polar orbits around cool stars. WASP-107b is also the fourth such planet to have a known distant planetary companion. We examined several dynamical pathways by which this companion could have induced such an obliquity in WASP-107b. We find that nodal precession and disk dispersal-driven tilting can both explain the current orbital geometry while Kozai-Lidov cycles are suppressed by general relativity. While each hypothesis requires a mutual inclination between the two planets, nodal precession requires a much larger angle, which for WASP-107 is on the threshold of detectability with future Gaia...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/39c8w4h4</guid>
      <pubDate>Thu, 5 Jan 2023 00:00:00 +0000</pubDate>
      <author>
        <name>Rubenzahl, Ryan A</name>
      </author>
      <author>
        <name>Dai, Fei</name>
      </author>
      <author>
        <name>Howard, Andrew W</name>
      </author>
      <author>
        <name>Chontos, Ashley</name>
      </author>
      <author>
        <name>Giacalone, Steven</name>
      </author>
      <author>
        <name>Lubin, Jack</name>
      </author>
      <author>
        <name>Rosenthal, Lee J</name>
      </author>
      <author>
        <name>Isaacson, Howard</name>
        <uri>https://orcid.org/0000-0002-0531-1073</uri>
      </author>
      <author>
        <name>Batalha, Natalie M</name>
      </author>
      <author>
        <name>Crossfield, Ian JM</name>
      </author>
      <author>
        <name>Dressing, Courtney</name>
        <uri>https://orcid.org/0000-0001-8189-0233</uri>
      </author>
      <author>
        <name>Fulton, Benjamin</name>
      </author>
      <author>
        <name>Huber, Daniel</name>
      </author>
      <author>
        <name>Kane, Stephen R</name>
        <uri>https://orcid.org/0000-0002-7084-0529</uri>
      </author>
      <author>
        <name>Petigura, Erik A</name>
      </author>
      <author>
        <name>Robertson, Paul</name>
      </author>
      <author>
        <name>Roy, Arpita</name>
      </author>
      <author>
        <name>Weiss, Lauren M</name>
      </author>
      <author>
        <name>Beard, Corey</name>
      </author>
      <author>
        <name>Hill, Michelle L</name>
      </author>
      <author>
        <name>Mayo, Andrew</name>
      </author>
      <author>
        <name>Mocnik, Teo</name>
      </author>
      <author>
        <name>Murphy, Joseph M Akana</name>
      </author>
      <author>
        <name>Scarsdale, Nicholas</name>
      </author>
    </item>
    <item>
      <title>Tentative Evidence for Water Vapor in the Atmosphere of the Neptune-Size Exoplanet HD 106315 c</title>
      <link>https://escholarship.org/uc/item/5rc965z8</link>
      <description>We present a transmission spectrum for the Neptune-size exoplanet HD 106315 c
from optical to infrared wavelengths based on transit observations from the
Hubble Space Telescope/Wide Field Camera 3, K2, and Spitzer. The spectrum shows
tentative evidence for a water absorption feature in the $1.1 - 1.7\mu$m
wavelength range with a small amplitude of 30 ppm (corresponding to just $0.8
\pm 0.04$ atmospheric scale heights). Based on an atmospheric retrieval
analysis, the presence of water vapor is tentatively favored with a Bayes
factor of 1.7 - 2.6 (depending on prior assumptions). The spectrum is most
consistent with either enhanced metallicity, high altitude condensates, or
both. Cloud-free solar composition atmospheres are ruled out at $&amp;gt;5\sigma$
confidence. We compare the spectrum to grids of cloudy and hazy forward models
and find that the spectrum is fit well by models with moderate cloud lofting or
haze formation efficiency, over a wide range of metallicities ($1 - 100\times$
solar)....</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/5rc965z8</guid>
      <pubDate>Wed, 4 Jan 2023 00:00:00 +0000</pubDate>
      <author>
        <name>Kreidberg, Laura</name>
      </author>
      <author>
        <name>Mollière, Paul</name>
      </author>
      <author>
        <name>Crossfield, Ian JM</name>
      </author>
      <author>
        <name>Thorngren, Daniel P</name>
      </author>
      <author>
        <name>Kawashima, Yui</name>
      </author>
      <author>
        <name>Morley, Caroline V</name>
      </author>
      <author>
        <name>Benneke, Björn</name>
      </author>
      <author>
        <name>Mikal-Evans, Thomas</name>
      </author>
      <author>
        <name>Berardo, David</name>
      </author>
      <author>
        <name>Kosiarek, Molly</name>
      </author>
      <author>
        <name>Gorjian, Varoujan</name>
      </author>
      <author>
        <name>Ciardi, David R</name>
      </author>
      <author>
        <name>Christiansen, Jessie L</name>
      </author>
      <author>
        <name>Dragomir, Diana</name>
      </author>
      <author>
        <name>Dressing, Courtney D</name>
      </author>
      <author>
        <name>Fortney, Jonathan J</name>
        <uri>https://orcid.org/0000-0002-9843-4354</uri>
      </author>
      <author>
        <name>Fulton, Benjamin J</name>
      </author>
      <author>
        <name>Greene, Thomas P</name>
      </author>
      <author>
        <name>Hardegree-Ullman, Kevin K</name>
      </author>
      <author>
        <name>Howard, Andrew W</name>
      </author>
      <author>
        <name>Howell, Steve B</name>
      </author>
      <author>
        <name>Isaacson, Howard</name>
        <uri>https://orcid.org/0000-0002-0531-1073</uri>
      </author>
      <author>
        <name>Krick, Jessica E</name>
      </author>
      <author>
        <name>Livingston, John H</name>
      </author>
      <author>
        <name>Lothringer, Joshua D</name>
      </author>
      <author>
        <name>Morales, Farisa Y</name>
      </author>
      <author>
        <name>Petigura, Erik A</name>
      </author>
      <author>
        <name>Rodriguez, Joseph E</name>
      </author>
      <author>
        <name>Schlieder, Joshua E</name>
      </author>
      <author>
        <name>Weiss, Lauren M</name>
      </author>
    </item>
    <item>
      <title>SDSS-IV MaNGA: How the Stellar Populations of Passive Central Galaxies Depend on Stellar and Halo Mass</title>
      <link>https://escholarship.org/uc/item/77f6c5hq</link>
      <description>We analyze spatially resolved and co-added SDSS-IV MaNGA spectra with signal-to-noise ratio ∼100 from 2200 passive central galaxies (z ∼ 0.05) to understand how central galaxy assembly depends on stellar mass (M *) and halo mass (M h ). We control for systematic errors in M h by employing a new group catalog from Tinker and the widely used Yang et al. catalog. At fixed M *, the strengths of several stellar absorption features vary systematically with M h . Completely model-free, this is one of the first indications that the stellar populations of centrals with identical M * are affected by the properties of their host halos. To interpret these variations, we applied full spectral fitting with the code alf. At fixed M *, centrals in more massive halos are older, show lower [Fe/H], and have higher [Mg/Fe] with 3.5σ confidence. We conclude that halos not only dictate how much M * galaxies assemble but also modulate their chemical enrichment histories. Turning to our analysis at fixed...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/77f6c5hq</guid>
      <pubDate>Fri, 16 Dec 2022 00:00:00 +0000</pubDate>
      <author>
        <name>Oyarzún, Grecco A</name>
      </author>
      <author>
        <name>Bundy, Kevin</name>
      </author>
      <author>
        <name>Westfall, Kyle B</name>
        <uri>https://orcid.org/0000-0003-1809-6920</uri>
      </author>
      <author>
        <name>Tinker, Jeremy L</name>
      </author>
      <author>
        <name>Belfiore, Francesco</name>
      </author>
      <author>
        <name>Argudo-Fernández, Maria</name>
      </author>
      <author>
        <name>Zheng, Zheng</name>
      </author>
      <author>
        <name>Conroy, Charlie</name>
      </author>
      <author>
        <name>Masters, Karen L</name>
      </author>
      <author>
        <name>Wake, David</name>
      </author>
      <author>
        <name>Law, David R</name>
      </author>
      <author>
        <name>McDermid, Richard M</name>
      </author>
      <author>
        <name>Aragón-Salamanca, Alfonso</name>
      </author>
      <author>
        <name>Parikh, Taniya</name>
      </author>
      <author>
        <name>Yan, Renbin</name>
      </author>
      <author>
        <name>Bershady, Matthew</name>
      </author>
      <author>
        <name>Sánchez, Sebastián F</name>
      </author>
      <author>
        <name>Andrews, Brett H</name>
      </author>
      <author>
        <name>Fernández-Trincado, José G</name>
      </author>
      <author>
        <name>Lane, Richard R</name>
      </author>
      <author>
        <name>Bizyaev, D</name>
      </author>
      <author>
        <name>Boardman, Nicholas Fraser</name>
      </author>
      <author>
        <name>Lacerna, Ivan</name>
      </author>
      <author>
        <name>Brownstein, JR</name>
      </author>
      <author>
        <name>Drory, Niv</name>
      </author>
      <author>
        <name>Zhang, Kai</name>
      </author>
    </item>
    <item>
      <title>The Need for Laboratory Measurements and Ab Initio Studies to Aid Understanding of Exoplanetary Atmospheres</title>
      <link>https://escholarship.org/uc/item/3db4r31q</link>
      <description>We are now on a clear trajectory for improvements in exoplanet observations
that will revolutionize our ability to characterize their atmospheric
structure, composition, and circulation, from gas giants to rocky planets.
However, exoplanet atmospheric models capable of interpreting the upcoming
observations are often limited by insufficiencies in the laboratory and
theoretical data that serve as critical inputs to atmospheric physical and
chemical tools. Here we provide an up-to-date and condensed description of
areas where laboratory and/or ab initio investigations could fill critical gaps
in our ability to model exoplanet atmospheric opacities, clouds, and chemistry,
building off a larger 2016 white paper, and endorsed by the NAS Exoplanet
Science Strategy report. Now is the ideal time for progress in these areas, but
this progress requires better access to, understanding of, and training in the
production of spectroscopic data as well as a better insight into chemical
reaction...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/3db4r31q</guid>
      <pubDate>Fri, 2 Sep 2022 00:00:00 +0000</pubDate>
      <author>
        <name>Fortney, Jonathan J</name>
        <uri>https://orcid.org/0000-0002-9843-4354</uri>
      </author>
      <author>
        <name>Robinson, Tyler D</name>
      </author>
      <author>
        <name>Domagal-Goldman, Shawn</name>
      </author>
      <author>
        <name>Genio, Anthony D Del</name>
      </author>
      <author>
        <name>Gordon, Iouli E</name>
      </author>
      <author>
        <name>Gharib-Nezhad, Ehsan</name>
      </author>
      <author>
        <name>Lewis, Nikole</name>
      </author>
      <author>
        <name>Sousa-Silva, Clara</name>
      </author>
      <author>
        <name>Airapetian, Vladimir</name>
      </author>
      <author>
        <name>Drouin, Brian</name>
      </author>
      <author>
        <name>Hargreaves, Robert J</name>
      </author>
      <author>
        <name>Huang, Xinchuan</name>
      </author>
      <author>
        <name>Karman, Tijs</name>
      </author>
      <author>
        <name>Ramirez, Ramses M</name>
      </author>
      <author>
        <name>Rieker, Gregory B</name>
      </author>
      <author>
        <name>Tennyson, Jonathan</name>
      </author>
      <author>
        <name>Wordsworth, Robin</name>
      </author>
      <author>
        <name>Yurchenko, Sergei N</name>
      </author>
      <author>
        <name>Johnson, Alexandria V</name>
      </author>
      <author>
        <name>Lee, Timothy J</name>
      </author>
      <author>
        <name>Dong, Chuanfei</name>
      </author>
      <author>
        <name>Kane, Stephen</name>
        <uri>https://orcid.org/0000-0002-7084-0529</uri>
      </author>
      <author>
        <name>Lopez-Morales, Mercedes</name>
      </author>
      <author>
        <name>Fauchez, Thomas</name>
      </author>
      <author>
        <name>Lee, Timothy</name>
      </author>
      <author>
        <name>Marley, Mark S</name>
      </author>
      <author>
        <name>Sung, Keeyoon</name>
      </author>
      <author>
        <name>Haghighipour, Nader</name>
      </author>
      <author>
        <name>Robinson, Tyler</name>
      </author>
      <author>
        <name>Horst, Sarah</name>
      </author>
      <author>
        <name>Gao, Peter</name>
      </author>
      <author>
        <name>Kao, Der-you</name>
      </author>
      <author>
        <name>Dressing, Courtney</name>
      </author>
      <author>
        <name>Lupu, Roxana</name>
      </author>
      <author>
        <name>Savin, Daniel Wolf</name>
      </author>
      <author>
        <name>Fleury, Benjamin</name>
      </author>
      <author>
        <name>Venot, Olivia</name>
      </author>
      <author>
        <name>Ascenzi, Daniela</name>
      </author>
      <author>
        <name>Milam, Stefanie</name>
      </author>
      <author>
        <name>Linnartz, Harold</name>
      </author>
      <author>
        <name>Gudipati, Murthy</name>
      </author>
      <author>
        <name>Gronoff, Guillaume</name>
      </author>
      <author>
        <name>Salama, Farid</name>
      </author>
      <author>
        <name>Gavilan, Lisseth</name>
      </author>
      <author>
        <name>Bouwman, Jordy</name>
      </author>
      <author>
        <name>Turbet, Martin</name>
      </author>
      <author>
        <name>Benilan, Yves</name>
      </author>
      <author>
        <name>Henderson, Bryana</name>
      </author>
      <author>
        <name>Batalha, Natalie</name>
      </author>
      <author>
        <name>Jensen-Clem, Rebecca</name>
      </author>
      <author>
        <name>Lyons, Timothy</name>
      </author>
      <author>
        <name>Freedman, Richard</name>
      </author>
      <author>
        <name>Schwieterman, Edward</name>
        <uri>https://orcid.org/0000-0002-2949-2163</uri>
      </author>
      <author>
        <name>Goyal, Jayesh</name>
      </author>
      <author>
        <name>Mancini, Luigi</name>
      </author>
      <author>
        <name>Irwin, Patrick</name>
      </author>
      <author>
        <name>Desert, Jean-Michel</name>
      </author>
      <author>
        <name>Molaverdikhani, Karan</name>
      </author>
      <author>
        <name>Gizis, John</name>
      </author>
      <author>
        <name>Taylor, Jake</name>
      </author>
      <author>
        <name>Lothringer, Joshua</name>
      </author>
      <author>
        <name>Pierrehumbert, Raymond</name>
      </author>
      <author>
        <name>Zellem, Robert</name>
      </author>
      <author>
        <name>Batalha, Natasha</name>
      </author>
      <author>
        <name>Rugheimer, Sarah</name>
      </author>
      <author>
        <name>Lustig-Yaeger, Jacob</name>
      </author>
      <author>
        <name>Hu, Renyu</name>
      </author>
      <author>
        <name>Kempton, Eliza</name>
      </author>
      <author>
        <name>Arney, Giada</name>
      </author>
      <author>
        <name>Line, Mike</name>
      </author>
      <author>
        <name>Alam, Munazza</name>
      </author>
      <author>
        <name>Moses, Julianne</name>
      </author>
      <author>
        <name>Iro, Nicolas</name>
      </author>
      <author>
        <name>Kreidberg, Laura</name>
      </author>
      <author>
        <name>Blecic, Jasmina</name>
      </author>
      <author>
        <name>Louden, Tom</name>
      </author>
      <author>
        <name>Molliere, Paul</name>
      </author>
      <author>
        <name>Stevenson, Kevin</name>
      </author>
      <author>
        <name>Swain, Mark</name>
      </author>
      <author>
        <name>Bott, Kimberly</name>
      </author>
      <author>
        <name>Madhusudhan, Nikku</name>
      </author>
      <author>
        <name>Krissansen-Totton, Joshua</name>
      </author>
      <author>
        <name>Deming, Drake</name>
      </author>
      <author>
        <name>Kitiashvili, Irina</name>
      </author>
      <author>
        <name>Shkolnik, Evgenya</name>
      </author>
      <author>
        <name>Rustamkulov, Zafar</name>
      </author>
      <author>
        <name>Rogers, Leslie</name>
      </author>
      <author>
        <name>Close, Laird</name>
      </author>
    </item>
    <item>
      <title>Exoplanet Diversity in the Era of Space-based Direct Imaging Missions</title>
      <link>https://escholarship.org/uc/item/32x3m4f8</link>
      <description>This whitepaper discusses the diversity of exoplanets that could be detected
by future observations, so that comparative exoplanetology can be performed in
the upcoming era of large space-based flagship missions. The primary focus will
be on characterizing Earth-like worlds around Sun-like stars. However, we will
also be able to characterize companion planets in the system simultaneously.
This will not only provide a contextual picture with regards to our Solar
system, but also presents a unique opportunity to observe size dependent
planetary atmospheres at different orbital distances. We propose a preliminary
scheme based on chemical behavior of gases and condensates in a planet's
atmosphere that classifies them with respect to planetary radius and incident
stellar flux.</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/32x3m4f8</guid>
      <pubDate>Fri, 2 Sep 2022 00:00:00 +0000</pubDate>
      <author>
        <name>Kopparapu, Ravi</name>
      </author>
      <author>
        <name>Hebrard, Eric</name>
      </author>
      <author>
        <name>Belikov, Rus</name>
      </author>
      <author>
        <name>Batalha, Natalie M</name>
      </author>
      <author>
        <name>Mulders, Gijs D</name>
      </author>
      <author>
        <name>Stark, Chris</name>
      </author>
      <author>
        <name>Teal, Dillon</name>
      </author>
      <author>
        <name>Domagal-Goldman, Shawn</name>
      </author>
      <author>
        <name>Gelino, Dawn</name>
      </author>
      <author>
        <name>Mandell, Avi</name>
      </author>
      <author>
        <name>Roberge, Aki</name>
      </author>
      <author>
        <name>Rinehart, Stephen</name>
      </author>
      <author>
        <name>Kane, Stephen R</name>
        <uri>https://orcid.org/0000-0002-7084-0529</uri>
      </author>
      <author>
        <name>Hasegawa, Yasuhiro</name>
      </author>
      <author>
        <name>Henning, Wade</name>
      </author>
      <author>
        <name>Hicks, Brian</name>
      </author>
      <author>
        <name>Adibekyan, Vardan</name>
      </author>
      <author>
        <name>Schwieterman, Edward W</name>
        <uri>https://orcid.org/0000-0002-2949-2163</uri>
      </author>
      <author>
        <name>Kohler, Erika</name>
      </author>
      <author>
        <name>Teske, Johanna</name>
      </author>
      <author>
        <name>Hinkel, Natalie</name>
      </author>
      <author>
        <name>Nixon, Conor</name>
      </author>
      <author>
        <name>France, Kevin</name>
      </author>
      <author>
        <name>Danchi, William</name>
      </author>
      <author>
        <name>Haqq-Misra, Jacob</name>
      </author>
      <author>
        <name>Wolf, Eric T</name>
      </author>
      <author>
        <name>Guzewich, Scott D</name>
      </author>
      <author>
        <name>Charnay, Benjamin</name>
      </author>
      <author>
        <name>Arney, Giada</name>
      </author>
      <author>
        <name>Hartnett, Hilairy E</name>
      </author>
      <author>
        <name>Lopez, Eric D</name>
      </author>
      <author>
        <name>Minniti, Dante</name>
      </author>
      <author>
        <name>Renaud, Joe</name>
      </author>
      <author>
        <name>Airapetian, Vladimir</name>
      </author>
      <author>
        <name>Dong, Chuanfei</name>
      </author>
      <author>
        <name>Genio, Anthony D Del</name>
      </author>
      <author>
        <name>Trainer, Melissa</name>
      </author>
      <author>
        <name>Rau, Gioia</name>
      </author>
      <author>
        <name>Jensen, Adam</name>
      </author>
      <author>
        <name>Way, Michael</name>
      </author>
      <author>
        <name>Lisse, Carey M</name>
      </author>
      <author>
        <name>Lyra, Wladimir</name>
      </author>
      <author>
        <name>Marchis, Franck</name>
      </author>
      <author>
        <name>Jontof-Hutter, Daniel</name>
      </author>
      <author>
        <name>Young, Patrick</name>
      </author>
      <author>
        <name>Pierrehumbert, Ray</name>
      </author>
      <author>
        <name>Harman, Chester E</name>
      </author>
      <author>
        <name>Fortney, Jonathan</name>
        <uri>https://orcid.org/0000-0002-9843-4354</uri>
      </author>
      <author>
        <name>Moore, Bill</name>
      </author>
      <author>
        <name>Beckwith, Steven</name>
      </author>
      <author>
        <name>Shock, Everett</name>
      </author>
      <author>
        <name>Desch, Steve</name>
      </author>
      <author>
        <name>Mandt, Kathleen E</name>
      </author>
      <author>
        <name>Izenberg, Noam</name>
      </author>
      <author>
        <name>Ford, Eric B</name>
      </author>
      <author>
        <name>Curry, Shannon</name>
      </author>
      <author>
        <name>Scharf, Caleb</name>
      </author>
      <author>
        <name>Anbar, Ariel</name>
      </author>
    </item>
    <item>
      <title>A solar C/O and sub-solar metallicity in a hot Jupiter atmosphere</title>
      <link>https://escholarship.org/uc/item/50n981s6</link>
      <description>Measurements of the atmospheric carbon (C) and oxygen (O) relative to hydrogen (H) in hot Jupiters (relative to their host stars) provide insight into their formation location and subsequent orbital migration1,2. Hot Jupiters that form beyond the major volatile (H2O/CO/CO2) ice lines and subsequently migrate post disk-dissipation are predicted have atmospheric carbon-to-oxygen ratios (C/O) near 1 and subsolar metallicities2, whereas planets that migrate through the disk before dissipation are predicted to be heavily polluted by infalling O-rich icy planetesimals, resulting in C/O &amp;lt; 0.5 and super-solar metallicities1,2. Previous observations of hot Jupiters have been able to provide bounded constraints on either H2O (refs. 3–5) or CO (refs. 6,7), but not both for the same planet, leaving uncertain4 the true elemental C and O inventory and subsequent C/O and metallicity determinations. Here we report spectroscopic observations of a typical transiting hot Jupiter, WASP-77Ab. From...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/50n981s6</guid>
      <pubDate>Thu, 1 Sep 2022 00:00:00 +0000</pubDate>
      <author>
        <name>Line, Michael R</name>
      </author>
      <author>
        <name>Brogi, Matteo</name>
      </author>
      <author>
        <name>Bean, Jacob L</name>
      </author>
      <author>
        <name>Gandhi, Siddharth</name>
      </author>
      <author>
        <name>Zalesky, Joseph</name>
      </author>
      <author>
        <name>Parmentier, Vivien</name>
      </author>
      <author>
        <name>Smith, Peter</name>
      </author>
      <author>
        <name>Mace, Gregory N</name>
      </author>
      <author>
        <name>Mansfield, Megan</name>
      </author>
      <author>
        <name>Kempton, Eliza M-R</name>
      </author>
      <author>
        <name>Fortney, Jonathan J</name>
        <uri>https://orcid.org/0000-0002-9843-4354</uri>
      </author>
      <author>
        <name>Shkolnik, Evgenya</name>
      </author>
      <author>
        <name>Patience, Jennifer</name>
      </author>
      <author>
        <name>Rauscher, Emily</name>
      </author>
      <author>
        <name>Désert, Jean-Michel</name>
      </author>
      <author>
        <name>Wardenier, Joost P</name>
      </author>
    </item>
    <item>
      <title>The Seventeenth Data Release of the Sloan Digital Sky Surveys: Complete Release of MaNGA, MaStar, and APOGEE-2 Data</title>
      <link>https://escholarship.org/uc/item/2qw2m22g</link>
      <description>This paper documents the seventeenth data release (DR17) from the Sloan Digital Sky Surveys; the fifth and final release from the fourth phase (SDSS-IV). DR17 contains the complete release of the Mapping Nearby Galaxies at Apache Point Observatory (MaNGA) survey, which reached its goal of surveying over 10,000 nearby galaxies. The complete release of the MaNGA Stellar Library accompanies this data, providing observations of almost 30,000 stars through the MaNGA instrument during bright time. DR17 also contains the complete release of the Apache Point Observatory Galactic Evolution Experiment 2 survey that publicly releases infrared spectra of over 650,000 stars. The main sample from the Extended Baryon Oscillation Spectroscopic Survey (eBOSS), as well as the subsurvey Time Domain Spectroscopic Survey data were fully released in DR16. New single-fiber optical spectroscopy released in DR17 is from the SPectroscipic IDentification of ERosita Survey subsurvey and the eBOSS-RM program....</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/2qw2m22g</guid>
      <pubDate>Wed, 24 Aug 2022 00:00:00 +0000</pubDate>
      <author>
        <name>Abdurro’uf</name>
      </author>
      <author>
        <name>Accetta, Katherine</name>
      </author>
      <author>
        <name>Aerts, Conny</name>
      </author>
      <author>
        <name>Aguirre, Víctor Silva</name>
      </author>
      <author>
        <name>Ahumada, Romina</name>
      </author>
      <author>
        <name>Ajgaonkar, Nikhil</name>
      </author>
      <author>
        <name>Ak, N Filiz</name>
      </author>
      <author>
        <name>Alam, Shadab</name>
      </author>
      <author>
        <name>Prieto, Carlos Allende</name>
      </author>
      <author>
        <name>Almeida, Andrés</name>
      </author>
      <author>
        <name>Anders, Friedrich</name>
      </author>
      <author>
        <name>Anderson, Scott F</name>
      </author>
      <author>
        <name>Andrews, Brett H</name>
      </author>
      <author>
        <name>Anguiano, Borja</name>
      </author>
      <author>
        <name>Aquino-Ortíz, Erik</name>
      </author>
      <author>
        <name>Aragón-Salamanca, Alfonso</name>
      </author>
      <author>
        <name>Argudo-Fernández, Maria</name>
      </author>
      <author>
        <name>Ata, Metin</name>
      </author>
      <author>
        <name>Aubert, Marie</name>
      </author>
      <author>
        <name>Avila-Reese, Vladimir</name>
      </author>
      <author>
        <name>Badenes, Carles</name>
      </author>
      <author>
        <name>Barbá, Rodolfo H</name>
      </author>
      <author>
        <name>Barger, Kat</name>
      </author>
      <author>
        <name>Barrera-Ballesteros, Jorge K</name>
      </author>
      <author>
        <name>Beaton, Rachael L</name>
      </author>
      <author>
        <name>Beers, Timothy C</name>
      </author>
      <author>
        <name>Belfiore, Francesco</name>
      </author>
      <author>
        <name>Bender, Chad F</name>
      </author>
      <author>
        <name>Bernardi, Mariangela</name>
      </author>
      <author>
        <name>Bershady, Matthew A</name>
      </author>
      <author>
        <name>Beutler, Florian</name>
      </author>
      <author>
        <name>Bidin, Christian Moni</name>
      </author>
      <author>
        <name>Bird, Jonathan C</name>
      </author>
      <author>
        <name>Bizyaev, Dmitry</name>
      </author>
      <author>
        <name>Blanc, Guillermo A</name>
      </author>
      <author>
        <name>Blanton, Michael R</name>
      </author>
      <author>
        <name>Boardman, Nicholas Fraser</name>
      </author>
      <author>
        <name>Bolton, Adam S</name>
      </author>
      <author>
        <name>Boquien, Médéric</name>
      </author>
      <author>
        <name>Borissova, Jura</name>
      </author>
      <author>
        <name>Bovy, Jo</name>
      </author>
      <author>
        <name>Brandt, WN</name>
      </author>
      <author>
        <name>Brown, Jordan</name>
      </author>
      <author>
        <name>Brownstein, Joel R</name>
      </author>
      <author>
        <name>Brusa, Marcella</name>
      </author>
      <author>
        <name>Buchner, Johannes</name>
      </author>
      <author>
        <name>Bundy, Kevin</name>
      </author>
      <author>
        <name>Burchett, Joseph N</name>
      </author>
      <author>
        <name>Bureau, Martin</name>
      </author>
      <author>
        <name>Burgasser, Adam</name>
        <uri>https://orcid.org/0000-0002-6523-9536</uri>
      </author>
      <author>
        <name>Cabang, Tuesday K</name>
      </author>
      <author>
        <name>Campbell, Stephanie</name>
      </author>
      <author>
        <name>Cappellari, Michele</name>
      </author>
      <author>
        <name>Carlberg, Joleen K</name>
      </author>
      <author>
        <name>Wanderley, Fábio Carneiro</name>
      </author>
      <author>
        <name>Carrera, Ricardo</name>
      </author>
      <author>
        <name>Cash, Jennifer</name>
      </author>
      <author>
        <name>Chen, Yan-Ping</name>
      </author>
      <author>
        <name>Chen, Wei-Huai</name>
      </author>
      <author>
        <name>Cherinka, Brian</name>
      </author>
      <author>
        <name>Chiappini, Cristina</name>
      </author>
      <author>
        <name>Choi, Peter Doohyun</name>
      </author>
      <author>
        <name>Chojnowski, S Drew</name>
      </author>
      <author>
        <name>Chung, Haeun</name>
      </author>
      <author>
        <name>Clerc, Nicolas</name>
      </author>
      <author>
        <name>Cohen, Roger E</name>
      </author>
      <author>
        <name>Comerford, Julia M</name>
      </author>
      <author>
        <name>Comparat, Johan</name>
      </author>
      <author>
        <name>da Costa, Luiz</name>
      </author>
      <author>
        <name>Covey, Kevin</name>
      </author>
      <author>
        <name>Crane, Jeffrey D</name>
      </author>
      <author>
        <name>Cruz-Gonzalez, Irene</name>
      </author>
      <author>
        <name>Culhane, Connor</name>
      </author>
      <author>
        <name>Cunha, Katia</name>
      </author>
      <author>
        <name>Dai, Y Sophia</name>
      </author>
      <author>
        <name>Damke, Guillermo</name>
      </author>
      <author>
        <name>Darling, Jeremy</name>
      </author>
      <author>
        <name>Davidson, James W</name>
      </author>
      <author>
        <name>Davies, Roger</name>
      </author>
      <author>
        <name>Dawson, Kyle</name>
      </author>
      <author>
        <name>De Lee, Nathan</name>
      </author>
      <author>
        <name>Diamond-Stanic, Aleksandar M</name>
      </author>
      <author>
        <name>Cano-Díaz, Mariana</name>
      </author>
      <author>
        <name>Sánchez, Helena Domínguez</name>
      </author>
      <author>
        <name>Donor, John</name>
      </author>
      <author>
        <name>Duckworth, Chris</name>
      </author>
      <author>
        <name>Dwelly, Tom</name>
      </author>
      <author>
        <name>Eisenstein, Daniel J</name>
      </author>
      <author>
        <name>Elsworth, Yvonne P</name>
      </author>
      <author>
        <name>Emsellem, Eric</name>
      </author>
      <author>
        <name>Eracleous, Mike</name>
      </author>
      <author>
        <name>Escoffier, Stephanie</name>
      </author>
      <author>
        <name>Fan, Xiaohui</name>
      </author>
      <author>
        <name>Farr, Emily</name>
      </author>
      <author>
        <name>Feng, Shuai</name>
      </author>
      <author>
        <name>Fernández-Trincado, José G</name>
      </author>
      <author>
        <name>Feuillet, Diane</name>
      </author>
      <author>
        <name>Filipp, Andreas</name>
      </author>
      <author>
        <name>Fillingham, Sean P</name>
      </author>
      <author>
        <name>Frinchaboy, Peter M</name>
      </author>
    </item>
    <item>
      <title>The case and context for atmospheric methane as an exoplanet biosignature</title>
      <link>https://escholarship.org/uc/item/4f99s0jf</link>
      <description>Methane has been proposed as an exoplanet biosignature. Imminent observations with the James Webb Space Telescope may enable methane detections on potentially habitable exoplanets, so it is essential to assess in what planetary contexts methane is a compelling biosignature. Methane’s short photochemical lifetime in terrestrial planet atmospheres implies that abundant methane requires large replenishment fluxes. While methane can be produced by a variety of abiotic mechanisms such as outgassing, serpentinizing reactions, and impacts, we argue that—in contrast to an Earth-like biosphere—known abiotic processes cannot easily generate atmospheres rich in CH4 and CO2 with limited CO due to the strong redox disequilibrium between CH4 and CO2. Methane is thus more likely to be biogenic for planets with 1) a terrestrial bulk density, high mean-molecular-weight and anoxic atmosphere, and an old host star; 2) an abundance of CH4 that implies surface fluxes exceeding what could be supplied...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/4f99s0jf</guid>
      <pubDate>Fri, 22 Jul 2022 00:00:00 +0000</pubDate>
      <author>
        <name>Thompson, Maggie A</name>
      </author>
      <author>
        <name>Krissansen-Totton, Joshua</name>
      </author>
      <author>
        <name>Wogan, Nicholas</name>
      </author>
      <author>
        <name>Telus, Myriam</name>
      </author>
      <author>
        <name>Fortney, Jonathan J</name>
        <uri>https://orcid.org/0000-0002-9843-4354</uri>
      </author>
    </item>
    <item>
      <title>Final Targeting Strategy for the Sloan Digital Sky Survey IV Apache Point Observatory Galactic Evolution Experiment 2 North Survey</title>
      <link>https://escholarship.org/uc/item/4058w3z1</link>
      <description>The Apache Point Observatory Galactic Evolution Experiment 2 (APOGEE-2) is a dual-hemisphere, near-infrared (NIR), spectroscopic survey with the goal of producing a chemodynamical mapping of the Milky Way. The targeting for APOGEE-2 is complex and has evolved with time. In this paper, we present the updates and additions to the initial targeting strategy for APOGEE-2N presented in Zasowski et al. (2017). These modifications come in two implementation modes: (i) “Ancillary Science Programs” competitively awarded to Sloan Digital Sky Survey IV PIs through proposal calls in 2015 and 2017 for the pursuit of new scientific avenues outside the main survey, and (ii) an effective 1.5 yr expansion of the survey, known as the Bright Time Extension (BTX), made possible through accrued efficiency gains over the first years of the APOGEE-2N project. For the 23 distinct ancillary programs, we provide descriptions of the scientific aims, target selection, and how to identify these targets within...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/4058w3z1</guid>
      <pubDate>Wed, 20 Apr 2022 00:00:00 +0000</pubDate>
      <author>
        <name>Beaton, Rachael L</name>
      </author>
      <author>
        <name>Oelkers, Ryan J</name>
      </author>
      <author>
        <name>Hayes, Christian R</name>
      </author>
      <author>
        <name>Covey, Kevin R</name>
      </author>
      <author>
        <name>Chojnowski, SD</name>
      </author>
      <author>
        <name>De Lee, Nathan</name>
      </author>
      <author>
        <name>Sobeck, Jennifer S</name>
      </author>
      <author>
        <name>Majewski, Steven R</name>
      </author>
      <author>
        <name>Cohen, Roger E</name>
      </author>
      <author>
        <name>Fernández-Trincado, José</name>
      </author>
      <author>
        <name>Longa-Peña, Penélope</name>
      </author>
      <author>
        <name>O’Connell, Julia E</name>
      </author>
      <author>
        <name>Santana, Felipe A</name>
      </author>
      <author>
        <name>Stringfellow, Guy S</name>
      </author>
      <author>
        <name>Zasowski, Gail</name>
      </author>
      <author>
        <name>Aerts, Conny</name>
      </author>
      <author>
        <name>Anguiano, Borja</name>
      </author>
      <author>
        <name>Bender, Chad</name>
      </author>
      <author>
        <name>Cañas, Caleb I</name>
      </author>
      <author>
        <name>Cunha, Katia</name>
      </author>
      <author>
        <name>Donor, John</name>
      </author>
      <author>
        <name>Fleming, Scott W</name>
      </author>
      <author>
        <name>Frinchaboy, Peter M</name>
      </author>
      <author>
        <name>Feuillet, Diane</name>
      </author>
      <author>
        <name>Harding, Paul</name>
      </author>
      <author>
        <name>Hasselquist, Sten</name>
      </author>
      <author>
        <name>Holtzman, Jon A</name>
      </author>
      <author>
        <name>Johnson, Jennifer A</name>
      </author>
      <author>
        <name>Kollmeier, Juna A</name>
      </author>
      <author>
        <name>Kounkel, Marina</name>
      </author>
      <author>
        <name>Mahadevan, Suvrath</name>
      </author>
      <author>
        <name>Price-Whelan, Adrian M</name>
      </author>
      <author>
        <name>Rojas-Arriagada, Alvaro</name>
      </author>
      <author>
        <name>Román-Zúñiga, Carlos</name>
      </author>
      <author>
        <name>Schlafly, Edward F</name>
        <uri>https://orcid.org/0000-0002-3569-7421</uri>
      </author>
      <author>
        <name>Schultheis, Mathias</name>
      </author>
      <author>
        <name>Shetrone, Matthew</name>
        <uri>https://orcid.org/0000-0003-0509-2656</uri>
      </author>
      <author>
        <name>Simon, Joshua D</name>
      </author>
      <author>
        <name>Stassun, Keivan G</name>
      </author>
      <author>
        <name>Stutz, Amelia M</name>
      </author>
      <author>
        <name>Tayar, Jamie</name>
      </author>
      <author>
        <name>Teske, Johanna</name>
      </author>
      <author>
        <name>Tkachenko, Andrew</name>
      </author>
      <author>
        <name>Troup, Nicholas</name>
      </author>
      <author>
        <name>Albareti, Franco D</name>
      </author>
      <author>
        <name>Bizyaev, Dmitry</name>
      </author>
      <author>
        <name>Bovy, Jo</name>
      </author>
      <author>
        <name>Burgasser, Adam J</name>
        <uri>https://orcid.org/0000-0002-6523-9536</uri>
      </author>
      <author>
        <name>Comparat, Johan</name>
      </author>
      <author>
        <name>Downes, Juan José</name>
      </author>
      <author>
        <name>Geisler, Doug</name>
      </author>
      <author>
        <name>Inno, Laura</name>
      </author>
      <author>
        <name>Manchado, Arturo</name>
      </author>
      <author>
        <name>Ness, Melissa K</name>
      </author>
      <author>
        <name>Pinsonneault, Marc H</name>
      </author>
      <author>
        <name>Prada, Francisco</name>
      </author>
      <author>
        <name>Roman-Lopes, Alexandre</name>
      </author>
      <author>
        <name>Simonian, Gregory VA</name>
      </author>
      <author>
        <name>Smith, Verne V</name>
      </author>
      <author>
        <name>Yan, Renbin</name>
      </author>
      <author>
        <name>Zamora, Olga</name>
      </author>
    </item>
    <item>
      <title>The HETDEX Instrumentation: Hobby–Eberly Telescope Wide-field Upgrade and VIRUS</title>
      <link>https://escholarship.org/uc/item/4d77d3hk</link>
      <description>The Hobby–Eberly Telescope (HET) Dark Energy Experiment (HETDEX) is undertaking a blind wide-field low-resolution spectroscopic survey of 540 deg2 of sky to identify and derive redshifts for a million Lyα-emitting galaxies in the redshift range 1.9 &amp;lt; z &amp;lt; 3.5. The ultimate goal is to measure the expansion rate of the universe at this epoch, to sharply constrain cosmological parameters and thus the nature of dark energy. A major multiyear Wide-Field Upgrade (WFU) of the HET was completed in 2016 that substantially increased the field of view to 22′ diameter and the pupil to 10 m, by replacing the optical corrector, tracker, and Prime Focus Instrument Package and by developing a new telescope control system. The new, wide-field HET now feeds the Visible Integral-field Replicable Unit Spectrograph (VIRUS), a new low-resolution integral-field spectrograph (LRS2), and the Habitable Zone Planet Finder, a precision near-infrared radial velocity spectrograph. VIRUS consists of 156...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/4d77d3hk</guid>
      <pubDate>Tue, 19 Apr 2022 00:00:00 +0000</pubDate>
      <author>
        <name>Hill, Gary J</name>
      </author>
      <author>
        <name>Lee, Hanshin</name>
      </author>
      <author>
        <name>MacQueen, Phillip J</name>
      </author>
      <author>
        <name>Kelz, Andreas</name>
      </author>
      <author>
        <name>Drory, Niv</name>
      </author>
      <author>
        <name>Vattiat, Brian L</name>
      </author>
      <author>
        <name>Good, John M</name>
      </author>
      <author>
        <name>Ramsey, Jason</name>
      </author>
      <author>
        <name>Kriel, Herman</name>
      </author>
      <author>
        <name>Peterson, Trent</name>
      </author>
      <author>
        <name>DePoy, DL</name>
      </author>
      <author>
        <name>Gebhardt, Karl</name>
      </author>
      <author>
        <name>Marshall, JL</name>
      </author>
      <author>
        <name>Tuttle, Sarah E</name>
      </author>
      <author>
        <name>Bauer, Svend M</name>
      </author>
      <author>
        <name>Chonis, Taylor S</name>
      </author>
      <author>
        <name>Fabricius, Maximilian H</name>
      </author>
      <author>
        <name>Froning, Cynthia</name>
      </author>
      <author>
        <name>Häuser, Marco</name>
      </author>
      <author>
        <name>Indahl, Briana L</name>
      </author>
      <author>
        <name>Jahn, Thomas</name>
      </author>
      <author>
        <name>Landriau, Martin</name>
        <uri>https://orcid.org/0000-0003-1838-8528</uri>
      </author>
      <author>
        <name>Leck, Ron</name>
      </author>
      <author>
        <name>Montesano, Francesco</name>
      </author>
      <author>
        <name>Prochaska, Travis</name>
      </author>
      <author>
        <name>Snigula, Jan M</name>
      </author>
      <author>
        <name>Zeimann, Greg</name>
      </author>
      <author>
        <name>Bryant, Randy</name>
      </author>
      <author>
        <name>Damm, George</name>
      </author>
      <author>
        <name>Fowler, JR</name>
      </author>
      <author>
        <name>Janowiecki, Steven</name>
      </author>
      <author>
        <name>Martin, Jerry</name>
      </author>
      <author>
        <name>Mrozinski, Emily</name>
      </author>
      <author>
        <name>Odewahn, Stephen</name>
      </author>
      <author>
        <name>Rostopchin, Sergey</name>
      </author>
      <author>
        <name>Shetrone, Matthew</name>
        <uri>https://orcid.org/0000-0003-0509-2656</uri>
      </author>
      <author>
        <name>Spencer, Renny</name>
      </author>
      <author>
        <name>Cooper, Erin Mentuch</name>
      </author>
      <author>
        <name>Armandroff, Taft</name>
      </author>
      <author>
        <name>Bender, Ralf</name>
      </author>
      <author>
        <name>Dalton, Gavin</name>
      </author>
      <author>
        <name>Hopp, Ulrich</name>
      </author>
      <author>
        <name>Komatsu, Eiichiro</name>
      </author>
      <author>
        <name>Nicklas, Harald</name>
      </author>
      <author>
        <name>Ramsey, Lawrence W</name>
      </author>
      <author>
        <name>Roth, Martin M</name>
      </author>
      <author>
        <name>Schneider, Donald P</name>
      </author>
      <author>
        <name>Sneden, Chris</name>
      </author>
      <author>
        <name>Steinmetz, Matthias</name>
      </author>
    </item>
    <item>
      <title>The Hobby–Eberly Telescope Dark Energy Experiment (HETDEX) Survey Design, Reductions, and Detections* * Based on observations obtained with the Hobby–Eberly Telescope, which is a joint project of the University of Texas at Austin, the Pennsylvania State University, Ludwig-Maximilians-Universität München, and Georg-August-Universität Göttingen.</title>
      <link>https://escholarship.org/uc/item/38s3v07s</link>
      <description>We describe the survey design, calibration, commissioning, and emission-line detection algorithms for the Hobby–Eberly Telescope Dark Energy Experiment (HETDEX). The goal of HETDEX is to measure the redshifts of over a million Lyα emitting galaxies between 1.88 &amp;lt; z &amp;lt; 3.52, in a 540 deg2 area encompassing a comoving volume of 10.9 Gpc3. No preselection of targets is involved; instead the HETDEX measurements are accomplished via a spectroscopic survey using a suite of wide-field integral field units distributed over the focal plane of the telescope. This survey measures the Hubble expansion parameter and angular diameter distance, with a final expected accuracy of better than 1%. We detail the project’s observational strategy, reduction pipeline, source detection, and catalog generation, and present initial results for science verification in the Cosmological Evolution Survey, Extended Groth Strip, and Great Observatories Origins Deep Survey North fields. We demonstrate that...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/38s3v07s</guid>
      <pubDate>Tue, 19 Apr 2022 00:00:00 +0000</pubDate>
      <author>
        <name>Gebhardt, Karl</name>
      </author>
      <author>
        <name>Cooper, Erin Mentuch</name>
      </author>
      <author>
        <name>Ciardullo, Robin</name>
      </author>
      <author>
        <name>Acquaviva, Viviana</name>
      </author>
      <author>
        <name>Bender, Ralf</name>
      </author>
      <author>
        <name>Bowman, William P</name>
      </author>
      <author>
        <name>Castanheira, Barbara G</name>
      </author>
      <author>
        <name>Dalton, Gavin</name>
      </author>
      <author>
        <name>Davis, Dustin</name>
      </author>
      <author>
        <name>de Jong, Roelof S</name>
      </author>
      <author>
        <name>DePoy, DL</name>
      </author>
      <author>
        <name>Devarakonda, Yaswant</name>
      </author>
      <author>
        <name>Dongsheng, Sun</name>
      </author>
      <author>
        <name>Drory, Niv</name>
      </author>
      <author>
        <name>Fabricius, Maximilian</name>
      </author>
      <author>
        <name>Farrow, Daniel J</name>
      </author>
      <author>
        <name>Feldmeier, John</name>
      </author>
      <author>
        <name>Finkelstein, Steven L</name>
      </author>
      <author>
        <name>Froning, Cynthia S</name>
      </author>
      <author>
        <name>Gawiser, Eric</name>
      </author>
      <author>
        <name>Gronwall, Caryl</name>
      </author>
      <author>
        <name>Herold, Laura</name>
      </author>
      <author>
        <name>Hill, Gary J</name>
      </author>
      <author>
        <name>Hopp, Ulrich</name>
      </author>
      <author>
        <name>House, Lindsay R</name>
      </author>
      <author>
        <name>Janowiecki, Steven</name>
      </author>
      <author>
        <name>Jarvis, Matthew</name>
      </author>
      <author>
        <name>Jeong, Donghui</name>
      </author>
      <author>
        <name>Jogee, Shardha</name>
      </author>
      <author>
        <name>Kakuma, Ryota</name>
      </author>
      <author>
        <name>Kelz, Andreas</name>
      </author>
      <author>
        <name>Kollatschny, W</name>
      </author>
      <author>
        <name>Komatsu, Eiichiro</name>
      </author>
      <author>
        <name>Krumpe, Mirko</name>
      </author>
      <author>
        <name>Landriau, Martin</name>
        <uri>https://orcid.org/0000-0003-1838-8528</uri>
      </author>
      <author>
        <name>Liu, Chenxu</name>
      </author>
      <author>
        <name>Niemeyer, Maja Lujan</name>
      </author>
      <author>
        <name>MacQueen, Phillip</name>
      </author>
      <author>
        <name>Marshall, Jennifer</name>
      </author>
      <author>
        <name>Mawatari, Ken</name>
      </author>
      <author>
        <name>McLinden, Emily M</name>
      </author>
      <author>
        <name>Mukae, Shiro</name>
      </author>
      <author>
        <name>Nagaraj, Gautam</name>
      </author>
      <author>
        <name>Ono, Yoshiaki</name>
      </author>
      <author>
        <name>Ouchi, Masami</name>
      </author>
      <author>
        <name>Papovich, Casey</name>
      </author>
      <author>
        <name>Sakai, Nao</name>
      </author>
      <author>
        <name>Saito, Shun</name>
      </author>
      <author>
        <name>Schneider, Donald P</name>
      </author>
      <author>
        <name>Schulze, Andreas</name>
      </author>
      <author>
        <name>Shanmugasundararaj, Khavvia</name>
      </author>
      <author>
        <name>Shetrone, Matthew</name>
        <uri>https://orcid.org/0000-0003-0509-2656</uri>
      </author>
      <author>
        <name>Sneden, Chris</name>
      </author>
      <author>
        <name>Snigula, Jan</name>
      </author>
      <author>
        <name>Steinmetz, Matthias</name>
      </author>
      <author>
        <name>Thomas, Benjamin P</name>
      </author>
      <author>
        <name>Thomas, Brianna</name>
      </author>
      <author>
        <name>Tuttle, Sarah</name>
      </author>
      <author>
        <name>Urrutia, Tanya</name>
      </author>
      <author>
        <name>Wisotzki, Lutz</name>
      </author>
      <author>
        <name>Wold, Isak</name>
      </author>
      <author>
        <name>Zeimann, Gregory</name>
      </author>
      <author>
        <name>Zhang, Yechi</name>
      </author>
    </item>
    <item>
      <title>A tidal disruption event coincident with a high-energy neutrino</title>
      <link>https://escholarship.org/uc/item/3h76z2tp</link>
      <description>Cosmic neutrinos provide a unique window into the otherwise hidden mechanism of particle acceleration in astrophysical objects. The IceCube Collaboration recently reported the likely association of one high-energy neutrino with a flare from the relativistic jet of an active galaxy pointed towards the Earth. However a combined analysis of many similar active galaxies revealed no excess from the broader population, leaving the vast majority of the cosmic neutrino flux unexplained. Here we present the likely association of a radio-emitting tidal disruption event, AT2019dsg, with a second high-energy neutrino. AT2019dsg was identified as part of our systematic search for optical counterparts to high-energy neutrinos with the Zwicky Transient Facility. The probability of finding any coincident radio-emitting tidal disruption event by chance is 0.5%, while the probability of finding one as bright in bolometric energy flux as AT2019dsg is 0.2%. Our electromagnetic observations can be...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/3h76z2tp</guid>
      <pubDate>Mon, 20 Dec 2021 00:00:00 +0000</pubDate>
      <author>
        <name>Stein, Robert</name>
      </author>
      <author>
        <name>Velzen, Sjoert van</name>
      </author>
      <author>
        <name>Kowalski, Marek</name>
      </author>
      <author>
        <name>Franckowiak, Anna</name>
      </author>
      <author>
        <name>Gezari, Suvi</name>
      </author>
      <author>
        <name>Miller-Jones, James CA</name>
      </author>
      <author>
        <name>Frederick, Sara</name>
      </author>
      <author>
        <name>Sfaradi, Itai</name>
      </author>
      <author>
        <name>Bietenholz, Michael F</name>
      </author>
      <author>
        <name>Horesh, Assaf</name>
      </author>
      <author>
        <name>Fender, Rob</name>
      </author>
      <author>
        <name>Garrappa, Simone</name>
      </author>
      <author>
        <name>Ahumada, Tomás</name>
      </author>
      <author>
        <name>Andreoni, Igor</name>
      </author>
      <author>
        <name>Belicki, Justin</name>
      </author>
      <author>
        <name>Bellm, Eric C</name>
      </author>
      <author>
        <name>Böttcher, Markus</name>
      </author>
      <author>
        <name>Brinnel, Valery</name>
      </author>
      <author>
        <name>Burruss, Rick</name>
      </author>
      <author>
        <name>Cenko, S Bradley</name>
      </author>
      <author>
        <name>Coughlin, Michael W</name>
      </author>
      <author>
        <name>Cunningham, Virginia</name>
      </author>
      <author>
        <name>Drake, Andrew</name>
      </author>
      <author>
        <name>Farrar, Glennys R</name>
      </author>
      <author>
        <name>Feeney, Michael</name>
      </author>
      <author>
        <name>Foley, Ryan J</name>
        <uri>https://orcid.org/0000-0002-2445-5275</uri>
      </author>
      <author>
        <name>Gal-Yam, Avishay</name>
      </author>
      <author>
        <name>Golkhou, V Zach</name>
      </author>
      <author>
        <name>Goobar, Ariel</name>
      </author>
      <author>
        <name>Graham, Matthew J</name>
      </author>
      <author>
        <name>Hammerstein, Erica</name>
      </author>
      <author>
        <name>Helou, George</name>
      </author>
      <author>
        <name>Hung, Tiara</name>
      </author>
      <author>
        <name>Kasliwal, Mansi M</name>
      </author>
      <author>
        <name>Kilpatrick, Charles D</name>
      </author>
      <author>
        <name>Kong, Albert KH</name>
      </author>
      <author>
        <name>Kupfer, Thomas</name>
      </author>
      <author>
        <name>Laher, Russ R</name>
      </author>
      <author>
        <name>Mahabal, Ashish A</name>
      </author>
      <author>
        <name>Masci, Frank J</name>
      </author>
      <author>
        <name>Necker, Jannis</name>
      </author>
      <author>
        <name>Nordin, Jakob</name>
      </author>
      <author>
        <name>Perley, Daniel A</name>
      </author>
      <author>
        <name>Rigault, Mickael</name>
      </author>
      <author>
        <name>Reusch, Simeon</name>
      </author>
      <author>
        <name>Rodriguez, Hector</name>
      </author>
      <author>
        <name>Rojas-Bravo, César</name>
      </author>
      <author>
        <name>Rusholme, Ben</name>
      </author>
      <author>
        <name>Shupe, David L</name>
      </author>
      <author>
        <name>Singer, Leo P</name>
      </author>
      <author>
        <name>Sollerman, Jesper</name>
      </author>
      <author>
        <name>Soumagnac, Maayane T</name>
      </author>
      <author>
        <name>Stern, Daniel</name>
      </author>
      <author>
        <name>Taggart, Kirsty</name>
      </author>
      <author>
        <name>van Santen, Jakob</name>
      </author>
      <author>
        <name>Ward, Charlotte</name>
      </author>
      <author>
        <name>Woudt, Patrick</name>
      </author>
      <author>
        <name>Yao, Yuhan</name>
      </author>
    </item>
    <item>
      <title>CANDELS Multi-wavelength Catalogs: Source Identification and Photometry in the CANDELS Extended Groth Strip</title>
      <link>https://escholarship.org/uc/item/54d8z4h9</link>
      <description>We present a 0.4-8 μm multi-wavelength photometric catalog in the Extended Groth Strip (EGS) field. This catalog is built on the Hubble Space Telescope (HST) WFC3 and ACS data from the Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey (CANDELS), and it incorporates the existing HST data from the All-wavelength Extended Groth strip International Survey (AEGIS) and the 3D-HST program. The catalog is based on detections in the F160W band reaching a depth of F160W = 26.62 AB (90% completeness, point sources). It includes the photometry for 41,457 objects over an area of ≈ 206 arcmin2 in the following bands: HST/ACS F606W and F814W; HST WFC3 F125W, F140W, and F160W; Canada-France-Hawaii Telescope (CFHT)/Megacam u∗, g′, r′, i′ and z′; CFHT/WIRCAM J, H, and K S; Mayall/NEWFIRM J1, J2, J3, H1, H2, and K; Spitzer IRAC 3.6, 4.5, 5.8, and 8.0 μm. We are also releasing value-added catalogs that provide robust photometric redshifts and stellar mass measurements. The catalogs are...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/54d8z4h9</guid>
      <pubDate>Tue, 14 Dec 2021 00:00:00 +0000</pubDate>
      <author>
        <name>Stefanon, Mauro</name>
      </author>
      <author>
        <name>Yan, Haojing</name>
      </author>
      <author>
        <name>Mobasher, Bahram</name>
      </author>
      <author>
        <name>Barro, Guillermo</name>
      </author>
      <author>
        <name>Donley, Jennifer L</name>
      </author>
      <author>
        <name>Fontana, Adriano</name>
      </author>
      <author>
        <name>Hemmati, Shoubaneh</name>
      </author>
      <author>
        <name>Koekemoer, Anton M</name>
      </author>
      <author>
        <name>Lee, BoMee</name>
      </author>
      <author>
        <name>Lee, Seong-Kook</name>
      </author>
      <author>
        <name>Nayyeri, Hooshang</name>
      </author>
      <author>
        <name>Peth, Michael</name>
      </author>
      <author>
        <name>Pforr, Janine</name>
      </author>
      <author>
        <name>Salvato, Mara</name>
      </author>
      <author>
        <name>Wiklind, Tommy</name>
      </author>
      <author>
        <name>Wuyts, Stijn</name>
      </author>
      <author>
        <name>Ashby, Matthew LN</name>
      </author>
      <author>
        <name>Castellano, Marco</name>
      </author>
      <author>
        <name>Conselice, Christopher J</name>
      </author>
      <author>
        <name>Cooper, Michael C</name>
        <uri>https://orcid.org/0000-0003-1371-6019</uri>
      </author>
      <author>
        <name>Cooray, Asantha R</name>
      </author>
      <author>
        <name>Dolch, Timothy</name>
      </author>
      <author>
        <name>Ferguson, Henry</name>
      </author>
      <author>
        <name>Galametz, Audrey</name>
      </author>
      <author>
        <name>Giavalisco, Mauro</name>
      </author>
      <author>
        <name>Guo, Yicheng</name>
      </author>
      <author>
        <name>Willner, Steven P</name>
      </author>
      <author>
        <name>Dickinson, Mark E</name>
      </author>
      <author>
        <name>Faber, Sandra M</name>
      </author>
      <author>
        <name>Fazio, Giovanni G</name>
      </author>
      <author>
        <name>Gardner, Jonathan P</name>
      </author>
      <author>
        <name>Gawiser, Eric</name>
      </author>
      <author>
        <name>Grazian, Andrea</name>
      </author>
      <author>
        <name>Grogin, Norman A</name>
      </author>
      <author>
        <name>Kocevski, Dale</name>
      </author>
      <author>
        <name>Koo, David C</name>
        <uri>https://orcid.org/0000-0003-3385-6799</uri>
      </author>
      <author>
        <name>Lee, Kyoung-Soo</name>
      </author>
      <author>
        <name>Lucas, Ray A</name>
      </author>
      <author>
        <name>McGrath, Elizabeth J</name>
      </author>
      <author>
        <name>Nandra, Kirpal</name>
      </author>
      <author>
        <name>Newman, Jeffrey A</name>
      </author>
      <author>
        <name>van der Wel, Arjen</name>
      </author>
    </item>
    <item>
      <title>A PANCHROMATIC VIEW OF THE RESTLESS SN 2009ip REVEALS THE EXPLOSIVE EJECTION OF A MASSIVE STAR ENVELOPE</title>
      <link>https://escholarship.org/uc/item/9ph804bp</link>
      <description>The double explosion of SN 2009ip in 2012 raises questions about our understanding of the late stages of massive star evolution. Here we present a comprehensive study of SN 2009ip during its remarkable rebrightenings. High-cadence photometric and spectroscopic observations from the GeV to the radio band obtained from a variety of ground-based and space facilities (including the Very Large Array, Swift, Fermi, Hubble Space Telescope, and XMM) constrain SN 2009ip to be a low energy (E ∼ 1050 erg for an ejecta mass ∼0.5 M) and asymmetric explosion in a complex medium shaped by multiple eruptions of the restless progenitor star. Most of the energy is radiated as a result of the shock breaking out through a dense shell of material located at ∼5 × 1014 cm with M ∼ 0.1 M, ejected by the precursor outburst ∼40 days before the major explosion. We interpret the NIR excess of emission as signature of material located further out, the origin of which has to be connected with documented mass-loss...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/9ph804bp</guid>
      <pubDate>Mon, 13 Dec 2021 00:00:00 +0000</pubDate>
      <author>
        <name>Margutti, R</name>
      </author>
      <author>
        <name>Milisavljevic, D</name>
      </author>
      <author>
        <name>Soderberg, AM</name>
      </author>
      <author>
        <name>Chornock, R</name>
        <uri>https://orcid.org/0000-0002-7706-5668</uri>
      </author>
      <author>
        <name>Zauderer, BA</name>
      </author>
      <author>
        <name>Murase, K</name>
      </author>
      <author>
        <name>Guidorzi, C</name>
      </author>
      <author>
        <name>Sanders, NE</name>
      </author>
      <author>
        <name>Kuin, P</name>
      </author>
      <author>
        <name>Fransson, C</name>
      </author>
      <author>
        <name>Levesque, EM</name>
      </author>
      <author>
        <name>Chandra, P</name>
      </author>
      <author>
        <name>Berger, E</name>
      </author>
      <author>
        <name>Bianco, FB</name>
      </author>
      <author>
        <name>Brown, PJ</name>
      </author>
      <author>
        <name>Challis, P</name>
      </author>
      <author>
        <name>Chatzopoulos, E</name>
      </author>
      <author>
        <name>Cheung, CC</name>
      </author>
      <author>
        <name>Choi, C</name>
      </author>
      <author>
        <name>Chomiuk, L</name>
      </author>
      <author>
        <name>Chugai, N</name>
      </author>
      <author>
        <name>Contreras, C</name>
      </author>
      <author>
        <name>Drout, MR</name>
      </author>
      <author>
        <name>Fesen, R</name>
      </author>
      <author>
        <name>Foley, RJ</name>
        <uri>https://orcid.org/0000-0002-2445-5275</uri>
      </author>
      <author>
        <name>Fong, W</name>
      </author>
      <author>
        <name>Friedman, AS</name>
      </author>
      <author>
        <name>Gall, C</name>
      </author>
      <author>
        <name>Gehrels, N</name>
      </author>
      <author>
        <name>Hjorth, J</name>
      </author>
      <author>
        <name>Hsiao, E</name>
      </author>
      <author>
        <name>Kirshner, R</name>
      </author>
      <author>
        <name>Im, M</name>
      </author>
      <author>
        <name>Leloudas, G</name>
      </author>
      <author>
        <name>Lunnan, R</name>
      </author>
      <author>
        <name>Marion, GH</name>
      </author>
      <author>
        <name>Martin, J</name>
      </author>
      <author>
        <name>Morrell, N</name>
      </author>
      <author>
        <name>Neugent, KF</name>
      </author>
      <author>
        <name>Omodei, N</name>
      </author>
      <author>
        <name>Phillips, MM</name>
      </author>
      <author>
        <name>Rest, A</name>
      </author>
      <author>
        <name>Silverman, JM</name>
      </author>
      <author>
        <name>Strader, J</name>
      </author>
      <author>
        <name>Stritzinger, MD</name>
      </author>
      <author>
        <name>Szalai, T</name>
      </author>
      <author>
        <name>Utterback, NB</name>
      </author>
      <author>
        <name>Vinko, J</name>
      </author>
      <author>
        <name>Wheeler, JC</name>
      </author>
      <author>
        <name>Arnett, D</name>
      </author>
      <author>
        <name>Campana, S</name>
      </author>
      <author>
        <name>Chevalier, R</name>
      </author>
      <author>
        <name>Ginsburg, A</name>
      </author>
      <author>
        <name>Kamble, A</name>
      </author>
      <author>
        <name>Roming, PWA</name>
      </author>
      <author>
        <name>Pritchard, T</name>
      </author>
      <author>
        <name>Stringfellow, G</name>
      </author>
    </item>
    <item>
      <title>ALMA and RATIR observations of GRB&amp;nbsp;131030A</title>
      <link>https://escholarship.org/uc/item/7vn2p1nq</link>
      <description>We report on the first open-use based Atacama Large Millimeter/submm Array (ALMA) 345 GHz observation for the late afterglow phase of GRB 131030A. The ALMA observation constrained a deep limit at 17.1 d for the afterglow and host galaxy. We also identified a faint submillimeter source (ALMA J2300-0522) near the GRB 131030A position. The deep limit at 345 GHz and multifrequency observations obtained using Swift and RATIR yielded forward-shock modeling with a two-dimensional relativistic hydrodynamic jet simulation and described X-ray excess in the afterglow. The excess was inconsistent with the synchrotron self-inverse Compton radiation from the forward shock. The host galaxy of GRB 131030A and optical counterpart of ALMA J2300-0522 were also identified in the Subaru image. Based on the deep ALMA limit for the host galaxy, the 3σ upper limits of IR luminosity and the star formation rate (SFR) are estimated as LIR &amp;lt; 1.11 × 1011 L⊙ and SFR &amp;lt;18.7 (M⊙ yr-1), respectively. Although...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/7vn2p1nq</guid>
      <pubDate>Mon, 13 Dec 2021 00:00:00 +0000</pubDate>
      <author>
        <name>Huang, Kuiyun</name>
      </author>
      <author>
        <name>Urata, Yuji</name>
      </author>
      <author>
        <name>Takahashi, Satoko</name>
      </author>
      <author>
        <name>Im, Myungshin</name>
      </author>
      <author>
        <name>Yu, Po-Chieh</name>
      </author>
      <author>
        <name>Choi, Changsu</name>
      </author>
      <author>
        <name>Butler, Nathaniel</name>
      </author>
      <author>
        <name>Watson, Alan M</name>
      </author>
      <author>
        <name>Kutyrev, Alexander</name>
      </author>
      <author>
        <name>Lee, William H</name>
      </author>
      <author>
        <name>Klein, Chris</name>
      </author>
      <author>
        <name>Fox, Ori D</name>
      </author>
      <author>
        <name>Littlejohns, Owen</name>
      </author>
      <author>
        <name>Cucchiara, Nino</name>
      </author>
      <author>
        <name>Troja, Eleonora</name>
      </author>
      <author>
        <name>González, Jesús</name>
      </author>
      <author>
        <name>Richer, Michael G</name>
      </author>
      <author>
        <name>Román-Zúñiga, Carlos</name>
      </author>
      <author>
        <name>Bloom, Josh</name>
      </author>
      <author>
        <name>Prochaska, J Xavier</name>
      </author>
      <author>
        <name>Gehrels, Neil</name>
      </author>
      <author>
        <name>Moseley, Harvey</name>
      </author>
      <author>
        <name>Georgiev, Leonid</name>
      </author>
      <author>
        <name>de Diego, José A</name>
      </author>
      <author>
        <name>Ramirez-Ruiz, Enrico</name>
      </author>
    </item>
    <item>
      <title>The Palomar Transient Factory Core-collapse Supernova Host-galaxy Sample. I. Host-galaxy Distribution Functions and Environment Dependence of Core-collapse Supernovae</title>
      <link>https://escholarship.org/uc/item/98c8s865</link>
      <description>Abstract  Several thousand core-collapse supernovae (CCSNe) of different flavors have been discovered so far. However, identifying their progenitors has remained an outstanding open question in astrophysics. Studies of SN host galaxies have proven to be powerful in providing constraints on the progenitor populations. In this paper, we present all CCSNe detected between 2009 and 2017 by the Palomar Transient Factory. This sample includes 888 SNe of 12 distinct classes out to redshift z ≈ 1. We present the photometric properties of their host galaxies from the far-ultraviolet to the mid-infrared and model the host-galaxy spectral energy distributions to derive physical properties. The galaxy mass function of Type Ic, Ib, IIb, II, and IIn SNe ranges from 10 5 to 10 11.5 M ⊙ , probing the entire mass range of star-forming galaxies down to the least-massive star-forming galaxies known. Moreover, the galaxy mass distributions are consistent with models of star-formation-weighted mass...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/98c8s865</guid>
      <pubDate>Mon, 13 Sep 2021 00:00:00 +0000</pubDate>
      <author>
        <name>Schulze, Steve</name>
      </author>
      <author>
        <name>Yaron, Ofer</name>
      </author>
      <author>
        <name>Sollerman, Jesper</name>
      </author>
      <author>
        <name>Leloudas, Giorgos</name>
      </author>
      <author>
        <name>Gal, Amit</name>
      </author>
      <author>
        <name>Wright, Angus H</name>
      </author>
      <author>
        <name>Lunnan, Ragnhild</name>
      </author>
      <author>
        <name>Gal-Yam, Avishay</name>
      </author>
      <author>
        <name>Ofek, Eran O</name>
      </author>
      <author>
        <name>Perley, Daniel A</name>
      </author>
      <author>
        <name>Filippenko, Alexei V</name>
        <uri>https://orcid.org/0000-0003-3460-0103</uri>
      </author>
      <author>
        <name>Kasliwal, Mansi M</name>
      </author>
      <author>
        <name>Kulkarni, Shrinivas R</name>
      </author>
      <author>
        <name>Neill, James D</name>
      </author>
      <author>
        <name>Nugent, Peter E</name>
        <uri>https://orcid.org/0000-0002-3389-0586</uri>
      </author>
      <author>
        <name>Quimby, Robert M</name>
      </author>
      <author>
        <name>Sullivan, Mark</name>
      </author>
      <author>
        <name>Strotjohann, Nora Linn</name>
      </author>
      <author>
        <name>Arcavi, Iair</name>
      </author>
      <author>
        <name>Ben-Ami, Sagi</name>
      </author>
      <author>
        <name>Bianco, Federica</name>
      </author>
      <author>
        <name>Bloom, Joshua S</name>
      </author>
      <author>
        <name>De, Kishalay</name>
      </author>
      <author>
        <name>Fraser, Morgan</name>
      </author>
      <author>
        <name>Fremling, Christoffer U</name>
      </author>
      <author>
        <name>Horesh, Assaf</name>
      </author>
      <author>
        <name>Johansson, Joel</name>
      </author>
      <author>
        <name>Kelly, Patrick L</name>
      </author>
      <author>
        <name>Knežević, Nikola</name>
      </author>
      <author>
        <name>Knežević, Sladjana</name>
      </author>
      <author>
        <name>Maguire, Kate</name>
      </author>
      <author>
        <name>Nyholm, Anders</name>
      </author>
      <author>
        <name>Papadogiannakis, Seméli</name>
      </author>
      <author>
        <name>Petrushevska, Tanja</name>
      </author>
      <author>
        <name>Rubin, Adam</name>
      </author>
      <author>
        <name>Yan, Lin</name>
      </author>
      <author>
        <name>Yang, Yi</name>
      </author>
      <author>
        <name>Adams, Scott M</name>
      </author>
      <author>
        <name>Bufano, Filomena</name>
      </author>
      <author>
        <name>Clubb, Kelsey I</name>
      </author>
      <author>
        <name>Foley, Ryan J</name>
        <uri>https://orcid.org/0000-0002-2445-5275</uri>
      </author>
      <author>
        <name>Green, Yoav</name>
      </author>
      <author>
        <name>Harmanen, Jussi</name>
      </author>
      <author>
        <name>Ho, Anna YQ</name>
      </author>
      <author>
        <name>Hook, Isobel M</name>
      </author>
      <author>
        <name>Hosseinzadeh, Griffin</name>
      </author>
      <author>
        <name>Howell, D Andrew</name>
      </author>
      <author>
        <name>Kong, Albert KH</name>
      </author>
      <author>
        <name>Kotak, Rubina</name>
      </author>
      <author>
        <name>Matheson, Thomas</name>
      </author>
      <author>
        <name>McCully, Curtis</name>
      </author>
      <author>
        <name>Milisavljevic, Dan</name>
      </author>
      <author>
        <name>Pan, Yen-Chen</name>
      </author>
      <author>
        <name>Poznanski, Dovi</name>
      </author>
      <author>
        <name>Shivvers, Isaac</name>
      </author>
      <author>
        <name>van Velzen, Sjoert</name>
      </author>
      <author>
        <name>Verbeek, Kars K</name>
      </author>
    </item>
    <item>
      <title>First Cosmology Results using Supernovae Ia from the Dark Energy Survey: Survey Overview, Performance, and Supernova Spectroscopy</title>
      <link>https://escholarship.org/uc/item/8dn0h822</link>
      <description>We present details on the observing strategy, data-processing techniques, and spectroscopic targeting algorithms for the first three years of operation for the Dark Energy Survey Supernova Program (DES-SN). This five-year program using the Dark Energy Camera mounted on the 4 m Blanco telescope in Chile was designed to discover and follow supernovae (SNe) Ia over a wide redshift range (0.05 &amp;lt; z &amp;lt; 1.2) to measure the equation-of-state parameter of dark energy. We describe the SN program in full: strategy, observations, data reduction, spectroscopic follow-up observations, and classification. From three seasons of data, we have discovered 12,015 likely SNe, 308 of which have been spectroscopically confirmed, including 251 SNe Ia over a redshift range of 0.017 &amp;lt; z &amp;lt; 0.85. We determine the effective spectroscopic selection function for our sample and use it to investigate the redshift-dependent bias on the distance moduli of SNe Ia we have classified. The data presented...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/8dn0h822</guid>
      <pubDate>Tue, 3 Aug 2021 00:00:00 +0000</pubDate>
      <author>
        <name>Smith, M</name>
      </author>
      <author>
        <name>D’Andrea, CB</name>
      </author>
      <author>
        <name>Sullivan, M</name>
      </author>
      <author>
        <name>Möller, A</name>
      </author>
      <author>
        <name>Nichol, RC</name>
      </author>
      <author>
        <name>Thomas, RC</name>
      </author>
      <author>
        <name>Kim, AG</name>
        <uri>https://orcid.org/0000-0001-6315-8743</uri>
      </author>
      <author>
        <name>Sako, M</name>
      </author>
      <author>
        <name>Castander, FJ</name>
      </author>
      <author>
        <name>Filippenko, AV</name>
        <uri>https://orcid.org/0000-0003-3460-0103</uri>
      </author>
      <author>
        <name>Foley, RJ</name>
        <uri>https://orcid.org/0000-0002-2445-5275</uri>
      </author>
      <author>
        <name>Galbany, L</name>
      </author>
      <author>
        <name>González-Gaitán, S</name>
      </author>
      <author>
        <name>Kasai, E</name>
      </author>
      <author>
        <name>Kirshner, RP</name>
      </author>
      <author>
        <name>Lidman, C</name>
      </author>
      <author>
        <name>Scolnic, D</name>
      </author>
      <author>
        <name>Brout, D</name>
      </author>
      <author>
        <name>Davis, TM</name>
      </author>
      <author>
        <name>Gupta, RR</name>
      </author>
      <author>
        <name>Hinton, SR</name>
      </author>
      <author>
        <name>Kessler, R</name>
      </author>
      <author>
        <name>Lasker, J</name>
      </author>
      <author>
        <name>Macaulay, E</name>
      </author>
      <author>
        <name>Wolf, RC</name>
      </author>
      <author>
        <name>Zhang, B</name>
      </author>
      <author>
        <name>Asorey, J</name>
      </author>
      <author>
        <name>Avelino, A</name>
      </author>
      <author>
        <name>Bassett, BA</name>
      </author>
      <author>
        <name>Calcino, J</name>
      </author>
      <author>
        <name>Carollo, D</name>
      </author>
      <author>
        <name>Casas, R</name>
      </author>
      <author>
        <name>Challis, P</name>
      </author>
      <author>
        <name>Childress, M</name>
      </author>
      <author>
        <name>Clocchiatti, A</name>
      </author>
      <author>
        <name>Crawford, S</name>
      </author>
      <author>
        <name>Frohmaier, C</name>
      </author>
      <author>
        <name>Glazebrook, K</name>
      </author>
      <author>
        <name>Goldstein, DA</name>
      </author>
      <author>
        <name>Graham, ML</name>
      </author>
      <author>
        <name>Hoormann, JK</name>
      </author>
      <author>
        <name>Kuehn, K</name>
      </author>
      <author>
        <name>Lewis, GF</name>
      </author>
      <author>
        <name>Mandel, KS</name>
      </author>
      <author>
        <name>Morganson, E</name>
      </author>
      <author>
        <name>Muthukrishna, D</name>
      </author>
      <author>
        <name>Nugent, P</name>
        <uri>https://orcid.org/0000-0002-3389-0586</uri>
      </author>
      <author>
        <name>Pan, Y-C</name>
      </author>
      <author>
        <name>Pursiainen, M</name>
      </author>
      <author>
        <name>Sharp, R</name>
      </author>
      <author>
        <name>Sommer, NE</name>
      </author>
      <author>
        <name>Swann, E</name>
      </author>
      <author>
        <name>Thomas, BP</name>
      </author>
      <author>
        <name>Tucker, BE</name>
      </author>
      <author>
        <name>Uddin, SA</name>
      </author>
      <author>
        <name>Wiseman, P</name>
      </author>
      <author>
        <name>Zheng, W</name>
      </author>
      <author>
        <name>Abbott, TMC</name>
      </author>
      <author>
        <name>Annis, J</name>
      </author>
      <author>
        <name>Avila, S</name>
      </author>
      <author>
        <name>Bechtol, K</name>
      </author>
      <author>
        <name>Bernstein, GM</name>
      </author>
      <author>
        <name>Bertin, E</name>
      </author>
      <author>
        <name>Brooks, D</name>
      </author>
      <author>
        <name>Burke, DL</name>
      </author>
      <author>
        <name>Rosell, A Carnero</name>
      </author>
      <author>
        <name>Kind, M Carrasco</name>
      </author>
      <author>
        <name>Carretero, J</name>
      </author>
      <author>
        <name>Cunha, CE</name>
      </author>
      <author>
        <name>da Costa, LN</name>
      </author>
      <author>
        <name>Davis, C</name>
      </author>
      <author>
        <name>De Vicente, J</name>
      </author>
      <author>
        <name>Diehl, HT</name>
      </author>
      <author>
        <name>Eifler, TF</name>
      </author>
      <author>
        <name>Estrada, J</name>
      </author>
      <author>
        <name>Frieman, J</name>
      </author>
      <author>
        <name>García-Bellido, J</name>
      </author>
      <author>
        <name>Gaztanaga, E</name>
      </author>
      <author>
        <name>Gerdes, DW</name>
      </author>
      <author>
        <name>Gruen, D</name>
      </author>
      <author>
        <name>Gruendl, RA</name>
      </author>
      <author>
        <name>Gschwend, J</name>
      </author>
      <author>
        <name>Gutierrez, G</name>
      </author>
      <author>
        <name>Hartley, WG</name>
      </author>
      <author>
        <name>Hollowood, DL</name>
      </author>
      <author>
        <name>Honscheid, K</name>
      </author>
      <author>
        <name>Hoyle, B</name>
      </author>
      <author>
        <name>James, DJ</name>
      </author>
      <author>
        <name>Johnson, MWG</name>
      </author>
      <author>
        <name>Johnson, MD</name>
      </author>
      <author>
        <name>Kuropatkin, N</name>
      </author>
      <author>
        <name>Li, TS</name>
      </author>
      <author>
        <name>Lima, M</name>
      </author>
      <author>
        <name>Maia, MAG</name>
      </author>
      <author>
        <name>March, M</name>
      </author>
      <author>
        <name>Marshall, JL</name>
      </author>
      <author>
        <name>Martini, P</name>
      </author>
      <author>
        <name>Menanteau, F</name>
      </author>
      <author>
        <name>Miller, CJ</name>
      </author>
      <author>
        <name>Miquel, R</name>
      </author>
    </item>
    <item>
      <title>AUTOMATED TRANSIENT IDENTIFICATION IN THE DARK ENERGY SURVEY</title>
      <link>https://escholarship.org/uc/item/5666j9q2</link>
      <description>We describe an algorithm for identifying point-source transients and moving objects on reference-subtracted optical images containing artifacts of processing and instrumentation. The algorithm makes use of the supervised machine learning technique known as Random Forest. We present results from its use in the Dark Energy Survey Supernova program (DES-SN), where it was trained using a sample of 898,963 signal and background events generated by the transient detection pipeline. After reprocessing the data collected during the first DES-SN observing season (2013 September through 2014 February) using the algorithm, the number of transient candidates eligible for human scanning decreased by a factor of 13.4, while only 1.0% of the artificial Type Ia supernovae (SNe) injected into search images to monitor survey efficiency were lost, most of which were very faint events. Here we characterize the algorithm’s performance in detail, and we discuss how it can inform pipeline design decisions...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/5666j9q2</guid>
      <pubDate>Tue, 3 Aug 2021 00:00:00 +0000</pubDate>
      <author>
        <name>Goldstein, DA</name>
      </author>
      <author>
        <name>D’Andrea, CB</name>
      </author>
      <author>
        <name>Fischer, JA</name>
      </author>
      <author>
        <name>Foley, RJ</name>
        <uri>https://orcid.org/0000-0002-2445-5275</uri>
      </author>
      <author>
        <name>Gupta, RR</name>
      </author>
      <author>
        <name>Kessler, R</name>
      </author>
      <author>
        <name>Kim, AG</name>
        <uri>https://orcid.org/0000-0001-6315-8743</uri>
      </author>
      <author>
        <name>Nichol, RC</name>
      </author>
      <author>
        <name>Nugent, PE</name>
        <uri>https://orcid.org/0000-0002-3389-0586</uri>
      </author>
      <author>
        <name>Papadopoulos, A</name>
      </author>
      <author>
        <name>Sako, M</name>
      </author>
      <author>
        <name>Smith, M</name>
      </author>
      <author>
        <name>Sullivan, M</name>
      </author>
      <author>
        <name>Thomas, RC</name>
      </author>
      <author>
        <name>Wester, W</name>
      </author>
      <author>
        <name>Wolf, RC</name>
      </author>
      <author>
        <name>Abdalla, FB</name>
      </author>
      <author>
        <name>Banerji, M</name>
      </author>
      <author>
        <name>Benoit-Lévy, A</name>
      </author>
      <author>
        <name>Bertin, E</name>
      </author>
      <author>
        <name>Brooks, D</name>
      </author>
      <author>
        <name>Rosell, A Carnero</name>
      </author>
      <author>
        <name>Castander, FJ</name>
      </author>
      <author>
        <name>da Costa, LN</name>
      </author>
      <author>
        <name>Covarrubias, R</name>
      </author>
      <author>
        <name>DePoy, DL</name>
      </author>
      <author>
        <name>Desai, S</name>
      </author>
      <author>
        <name>Diehl, HT</name>
      </author>
      <author>
        <name>Doel, P</name>
      </author>
      <author>
        <name>Eifler, TF</name>
      </author>
      <author>
        <name>Neto, A Fausti</name>
      </author>
      <author>
        <name>Finley, DA</name>
      </author>
      <author>
        <name>Flaugher, B</name>
      </author>
      <author>
        <name>Fosalba, P</name>
      </author>
      <author>
        <name>Frieman, J</name>
      </author>
      <author>
        <name>Gerdes, D</name>
      </author>
      <author>
        <name>Gruen, D</name>
      </author>
      <author>
        <name>Gruendl, RA</name>
      </author>
      <author>
        <name>James, D</name>
      </author>
      <author>
        <name>Kuehn, K</name>
      </author>
      <author>
        <name>Kuropatkin, N</name>
      </author>
      <author>
        <name>Lahav, O</name>
      </author>
      <author>
        <name>Li, TS</name>
      </author>
      <author>
        <name>Maia, MAG</name>
      </author>
      <author>
        <name>Makler, M</name>
      </author>
      <author>
        <name>March, M</name>
      </author>
      <author>
        <name>Marshall, JL</name>
      </author>
      <author>
        <name>Martini, P</name>
      </author>
      <author>
        <name>Merritt, KW</name>
      </author>
      <author>
        <name>Miquel, R</name>
      </author>
      <author>
        <name>Nord, B</name>
      </author>
      <author>
        <name>Ogando, R</name>
      </author>
      <author>
        <name>Plazas, AA</name>
      </author>
      <author>
        <name>Romer, AK</name>
      </author>
      <author>
        <name>Roodman, A</name>
      </author>
      <author>
        <name>Sanchez, E</name>
      </author>
      <author>
        <name>Scarpine, V</name>
      </author>
      <author>
        <name>Schubnell, M</name>
      </author>
      <author>
        <name>Sevilla-Noarbe, I</name>
      </author>
      <author>
        <name>Smith, RC</name>
      </author>
      <author>
        <name>Soares-Santos, M</name>
      </author>
      <author>
        <name>Sobreira, F</name>
      </author>
      <author>
        <name>Suchyta, E</name>
      </author>
      <author>
        <name>Swanson, MEC</name>
      </author>
      <author>
        <name>Tarle, G</name>
      </author>
      <author>
        <name>Thaler, J</name>
      </author>
      <author>
        <name>Walker, AR</name>
      </author>
    </item>
    <item>
      <title>iPTF14yb: THE FIRST DISCOVERY OF A GAMMA-RAY BURST AFTERGLOW INDEPENDENT OF A HIGH-ENERGY TRIGGER</title>
      <link>https://escholarship.org/uc/item/2qw8b8pm</link>
      <description>We report here the discovery by the Intermediate Palomar Transient Factory (iPTF) of iPTF14yb, a luminous ( mag), cosmological (redshift 1.9733), rapidly fading optical transient. We demonstrate, based on probabilistic arguments and a comparison with the broader population, that iPTF14yb is the optical afterglow of the long-duration gamma-ray burst GRB 140226A. This marks the first unambiguous discovery of a GRB afterglow prior to (and thus entirely independent of) an associated high-energy trigger. We estimate the rate of iPTF14yb-like sources (i.e., cosmologically distant relativistic explosions) based on iPTF observations, inferring an all-sky value of yr−1 (68% confidence interval of 110–2000 yr−1). Our derived rate is consistent (within the large uncertainty) with the all-sky rate of on-axis GRBs derived by the Swift satellite. Finally, we briefly discuss the implications of the nondetection to date of bona fide “orphan” afterglows (i.e., those lacking detectable high-energy...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/2qw8b8pm</guid>
      <pubDate>Tue, 3 Aug 2021 00:00:00 +0000</pubDate>
      <author>
        <name>Cenko, S Bradley</name>
      </author>
      <author>
        <name>Urban, Alex L</name>
      </author>
      <author>
        <name>Perley, Daniel A</name>
      </author>
      <author>
        <name>Horesh, Assaf</name>
      </author>
      <author>
        <name>Corsi, Alessandra</name>
      </author>
      <author>
        <name>Fox, Derek B</name>
      </author>
      <author>
        <name>Cao, Yi</name>
      </author>
      <author>
        <name>Kasliwal, Mansi M</name>
      </author>
      <author>
        <name>Lien, Amy</name>
      </author>
      <author>
        <name>Arcavi, Iair</name>
      </author>
      <author>
        <name>Bloom, Joshua S</name>
      </author>
      <author>
        <name>Butler, Nat R</name>
      </author>
      <author>
        <name>Cucchiara, Antonino</name>
      </author>
      <author>
        <name>de Diego, José A</name>
      </author>
      <author>
        <name>Filippenko, Alexei V</name>
        <uri>https://orcid.org/0000-0003-3460-0103</uri>
      </author>
      <author>
        <name>Gal-Yam, Avishay</name>
      </author>
      <author>
        <name>Gehrels, Neil</name>
      </author>
      <author>
        <name>Georgiev, Leonid</name>
      </author>
      <author>
        <name>González, J Jesús</name>
      </author>
      <author>
        <name>Graham, John F</name>
      </author>
      <author>
        <name>Greiner, Jochen</name>
      </author>
      <author>
        <name>Kann, D Alexander</name>
      </author>
      <author>
        <name>Klein, Christopher R</name>
      </author>
      <author>
        <name>Knust, Fabian</name>
      </author>
      <author>
        <name>Kulkarni, SR</name>
      </author>
      <author>
        <name>Kutyrev, Alexander</name>
      </author>
      <author>
        <name>Laher, Russ</name>
      </author>
      <author>
        <name>Lee, William H</name>
      </author>
      <author>
        <name>Nugent, Peter E</name>
        <uri>https://orcid.org/0000-0002-3389-0586</uri>
      </author>
      <author>
        <name>Prochaska, J Xavier</name>
      </author>
      <author>
        <name>Ramirez-Ruiz, Enrico</name>
        <uri>https://orcid.org/0000-0003-2558-3102</uri>
      </author>
      <author>
        <name>Richer, Michael G</name>
      </author>
      <author>
        <name>Rubin, Adam</name>
      </author>
      <author>
        <name>Urata, Yuji</name>
      </author>
      <author>
        <name>Varela, Karla</name>
      </author>
      <author>
        <name>Watson, Alan M</name>
      </author>
      <author>
        <name>Wozniak, Przemek R</name>
      </author>
    </item>
    <item>
      <title>DES13S2cmm: the first superluminous supernova from the Dark Energy Survey</title>
      <link>https://escholarship.org/uc/item/1n74360q</link>
      <description>We present DES13S2cmm, the first spectroscopically-confirmed superluminous supernova (SLSN) from the Dark Energy Survey (DES). We briefly discuss the data and search algorithm used to find this event in the first year of DES operations, and outline the spectroscopic data obtained from the European Southern Observatory (ESO) Very Large Telescope to confirm its redshift (z = 0.663 ± 0.001 based on the host-galaxy emission lines) and likely spectral type (Type I). Using this redshift, we find $M^{\rm peak}_U=-21.05^{+0.10}_{-0.09}$ for the peak, rest-frame U-band absolute magnitude, and find DES13S2cmm to be located in a faint, low-metallicity (sub-solar), low stellar-mass host galaxy (log (M/M⊙) = 9.3 ± 0.3), consistent with what is seen for other SLSNe-I. We compare the bolometric light curve of DES13S2cmm to 14 similarly well-observed SLSNe-I in the literature and find that it possesses one of the slowest declining tails (beyond +30 d rest-frame past peak), and is the faintest...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/1n74360q</guid>
      <pubDate>Tue, 3 Aug 2021 00:00:00 +0000</pubDate>
      <author>
        <name>Papadopoulos, A</name>
      </author>
      <author>
        <name>D'Andrea, CB</name>
      </author>
      <author>
        <name>Sullivan, M</name>
      </author>
      <author>
        <name>Nichol, RC</name>
      </author>
      <author>
        <name>Barbary, K</name>
      </author>
      <author>
        <name>Biswas, R</name>
      </author>
      <author>
        <name>Brown, PJ</name>
      </author>
      <author>
        <name>Covarrubias, RA</name>
      </author>
      <author>
        <name>Finley, DA</name>
      </author>
      <author>
        <name>Fischer, JA</name>
      </author>
      <author>
        <name>Foley, RJ</name>
        <uri>https://orcid.org/0000-0002-2445-5275</uri>
      </author>
      <author>
        <name>Goldstein, D</name>
      </author>
      <author>
        <name>Gupta, RR</name>
      </author>
      <author>
        <name>Kessler, R</name>
      </author>
      <author>
        <name>Kovacs, E</name>
      </author>
      <author>
        <name>Kuhlmann, SE</name>
      </author>
      <author>
        <name>Lidman, C</name>
      </author>
      <author>
        <name>March, M</name>
      </author>
      <author>
        <name>Nugent, PE</name>
        <uri>https://orcid.org/0000-0002-3389-0586</uri>
      </author>
      <author>
        <name>Sako, M</name>
      </author>
      <author>
        <name>Smith, RC</name>
      </author>
      <author>
        <name>Spinka, H</name>
      </author>
      <author>
        <name>Wester, W</name>
      </author>
      <author>
        <name>Abbott, TMC</name>
      </author>
      <author>
        <name>Abdalla, F</name>
      </author>
      <author>
        <name>Allam, SS</name>
      </author>
      <author>
        <name>Banerji, M</name>
      </author>
      <author>
        <name>Bernstein, JP</name>
      </author>
      <author>
        <name>Bernstein, RA</name>
      </author>
      <author>
        <name>Carnero, A</name>
      </author>
      <author>
        <name>da Costa, LN</name>
      </author>
      <author>
        <name>DePoy, DL</name>
      </author>
      <author>
        <name>Desai, S</name>
      </author>
      <author>
        <name>Diehl, HT</name>
      </author>
      <author>
        <name>Eifler, T</name>
      </author>
      <author>
        <name>Evrard, AE</name>
      </author>
      <author>
        <name>Flaugher, B</name>
      </author>
      <author>
        <name>Frieman, JA</name>
      </author>
      <author>
        <name>Gerdes, D</name>
      </author>
      <author>
        <name>Gruen, D</name>
      </author>
      <author>
        <name>Honscheid, K</name>
      </author>
      <author>
        <name>James, D</name>
      </author>
      <author>
        <name>Kuehn, K</name>
      </author>
      <author>
        <name>Kuropatkin, N</name>
      </author>
      <author>
        <name>Lahav, O</name>
      </author>
      <author>
        <name>Maia, MAG</name>
      </author>
      <author>
        <name>Makler, M</name>
      </author>
      <author>
        <name>Marshall, JL</name>
      </author>
      <author>
        <name>Merritt, KW</name>
      </author>
      <author>
        <name>Miller, CJ</name>
      </author>
      <author>
        <name>Miquel, R</name>
      </author>
      <author>
        <name>Ogando, R</name>
      </author>
      <author>
        <name>Plazas, AA</name>
      </author>
      <author>
        <name>Roe, NA</name>
      </author>
      <author>
        <name>Romer, AK</name>
      </author>
      <author>
        <name>Rykoff, E</name>
      </author>
      <author>
        <name>Sanchez, E</name>
      </author>
      <author>
        <name>Santiago, BX</name>
      </author>
      <author>
        <name>Scarpine, V</name>
      </author>
      <author>
        <name>Schubnell, M</name>
      </author>
      <author>
        <name>Sevilla, I</name>
      </author>
      <author>
        <name>Soares-Santos, M</name>
      </author>
      <author>
        <name>Suchyta, E</name>
      </author>
      <author>
        <name>Swanson, M</name>
      </author>
      <author>
        <name>Tarle, G</name>
      </author>
      <author>
        <name>Thaler, J</name>
      </author>
      <author>
        <name>Tucker, LD</name>
      </author>
      <author>
        <name>Wechsler, RH</name>
      </author>
      <author>
        <name>Zuntz, J</name>
      </author>
    </item>
    <item>
      <title>Astrophysics. Multiple images of a highly magnified supernova formed by an early-type cluster galaxy lens.</title>
      <link>https://escholarship.org/uc/item/05b81661</link>
      <description>In 1964, Refsdal hypothesized that a supernova whose light traversed multiple paths around a strong gravitational lens could be used to measure the rate of cosmic expansion. We report the discovery of such a system. In Hubble Space Telescope imaging, we have found four images of a single supernova forming an Einstein cross configuration around a redshift z = 0.54 elliptical galaxy in the MACS J1149.6+2223 cluster. The cluster's gravitational potential also creates multiple images of the z = 1.49 spiral supernova host galaxy, and a future appearance of the supernova elsewhere in the cluster field is expected. The magnifications and staggered arrivals of the supernova images probe the cosmic expansion rate, as well as the distribution of matter in the galaxy and cluster lenses.</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/05b81661</guid>
      <pubDate>Mon, 14 Jun 2021 00:00:00 +0000</pubDate>
      <author>
        <name>Kelly, Patrick L</name>
      </author>
      <author>
        <name>Rodney, Steven A</name>
        <uri>https://orcid.org/0000-0003-1947-687X</uri>
      </author>
      <author>
        <name>Treu, Tommaso</name>
        <uri>https://orcid.org/0000-0002-8460-0390</uri>
      </author>
      <author>
        <name>Foley, Ryan J</name>
        <uri>https://orcid.org/0000-0002-2445-5275</uri>
      </author>
      <author>
        <name>Brammer, Gabriel</name>
      </author>
      <author>
        <name>Schmidt, Kasper B</name>
        <uri>https://orcid.org/0000-0002-3418-7251</uri>
      </author>
      <author>
        <name>Zitrin, Adi</name>
        <uri>https://orcid.org/0000-0002-0350-4488</uri>
      </author>
      <author>
        <name>Sonnenfeld, Alessandro</name>
        <uri>https://orcid.org/0000-0002-6061-5977</uri>
      </author>
      <author>
        <name>Strolger, Louis-Gregory</name>
      </author>
      <author>
        <name>Graur, Or</name>
        <uri>https://orcid.org/0000-0002-4391-6137</uri>
      </author>
      <author>
        <name>Filippenko, Alexei V</name>
      </author>
      <author>
        <name>Jha, Saurabh W</name>
        <uri>https://orcid.org/0000-0001-8738-6011</uri>
      </author>
      <author>
        <name>Riess, Adam G</name>
      </author>
      <author>
        <name>Bradac, Marusa</name>
        <uri>https://orcid.org/0000-0001-5984-0395</uri>
      </author>
      <author>
        <name>Weiner, Benjamin J</name>
        <uri>https://orcid.org/0000-0001-6065-7483</uri>
      </author>
      <author>
        <name>Scolnic, Daniel</name>
      </author>
      <author>
        <name>Malkan, Matthew A</name>
        <uri>https://orcid.org/0000-0001-6919-1237</uri>
      </author>
      <author>
        <name>von der Linden, Anja</name>
      </author>
      <author>
        <name>Trenti, Michele</name>
        <uri>https://orcid.org/0000-0001-9391-305X</uri>
      </author>
      <author>
        <name>Hjorth, Jens</name>
      </author>
      <author>
        <name>Gavazzi, Raphael</name>
      </author>
      <author>
        <name>Fontana, Adriano</name>
        <uri>https://orcid.org/0000-0003-3820-2823</uri>
      </author>
      <author>
        <name>Merten, Julian C</name>
      </author>
      <author>
        <name>McCully, Curtis</name>
      </author>
      <author>
        <name>Jones, Tucker</name>
        <uri>https://orcid.org/0000-0001-5860-3419</uri>
      </author>
      <author>
        <name>Postman, Marc</name>
      </author>
      <author>
        <name>Dressler, Alan</name>
      </author>
      <author>
        <name>Patel, Brandon</name>
      </author>
      <author>
        <name>Cenko, S Bradley</name>
      </author>
      <author>
        <name>Graham, Melissa L</name>
        <uri>https://orcid.org/0000-0002-9154-3136</uri>
      </author>
      <author>
        <name>Tucker, Bradley E</name>
        <uri>https://orcid.org/0000-0002-4283-5159</uri>
      </author>
    </item>
    <item>
      <title>Performance of Kitt Peak’s Mayall 4-meter telescope during DESI commissioning</title>
      <link>https://escholarship.org/uc/item/9n74h9fq</link>
      <description>In preparation for the Dark Energy Spectroscopic Instrument (DESI), a new top end was installed on the Mayall 4-meter telescope at Kitt Peak National Observatory. The refurbished telescope and the DESI instrument were successfully commissioned on sky between 2019 October and 2020 March. Here we describe the pointing, tracking and imaging performance of the Mayall telescope equipped with its new DESI prime focus corrector, as measured by six guider cameras sampling the outer edge of DESI's focal plane. Analyzing ∼500,000 guider images acquired during commissioning, we find a median delivered image FWHM of 1.1 arcseconds (in the r-band at 650 nm), with the distribution extending to a best-case value of ∼0.6 arcseconds. The point spread function is well characterized by a Moffat profile with a power-law index of β ≈ 3.5 and little dependence of β on FWHM. The shape and size of the PSF delivered by the new corrector at a field angle of 1.57 degrees are very similar to those measured...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/9n74h9fq</guid>
      <pubDate>Wed, 17 Mar 2021 00:00:00 +0000</pubDate>
      <author>
        <name>Meisner, Aaron M</name>
      </author>
      <author>
        <name>Abareshi, Behzad</name>
      </author>
      <author>
        <name>Dey, Arjun</name>
      </author>
      <author>
        <name>Rockosi, Connie M</name>
      </author>
      <author>
        <name>Joyce, Richard R</name>
      </author>
      <author>
        <name>Sprayberry, David</name>
      </author>
      <author>
        <name>Besuner, Robert W</name>
      </author>
      <author>
        <name>Honscheid, Klaus</name>
      </author>
      <author>
        <name>Kirkby, David P</name>
        <uri>https://orcid.org/0000-0002-8828-5463</uri>
      </author>
      <author>
        <name>Kong, Hui</name>
      </author>
      <author>
        <name>Landriau, Martin</name>
      </author>
      <author>
        <name>Levi, Michael E</name>
      </author>
      <author>
        <name>Li, Ting S</name>
      </author>
      <author>
        <name>Marshall, Bob</name>
      </author>
      <author>
        <name>Martini, Paul</name>
      </author>
      <author>
        <name>Ross, Ashley J</name>
      </author>
      <author>
        <name>Brooks, David</name>
      </author>
      <author>
        <name>Doel, Peter</name>
      </author>
      <author>
        <name>Duan, Yutong</name>
      </author>
      <author>
        <name>Gaztanaga, Enrique</name>
      </author>
      <author>
        <name>Magneville, Christophe</name>
      </author>
      <author>
        <name>Prada, Francisco</name>
      </author>
      <author>
        <name>Schubnell, Michael</name>
      </author>
      <author>
        <name>Tarle, Gregory</name>
      </author>
    </item>
    <item>
      <title>Transmission Spectroscopy for the Warm Sub-Neptune HD 3167c: Evidence for Molecular Absorption and a Possible High-metallicity Atmosphere</title>
      <link>https://escholarship.org/uc/item/8bg71322</link>
      <description>We present a transmission spectrum for the warm (500-600 K) sub-Neptune HD 3167c obtained using the Hubble Space Telescope Wide Field Camera 3 infrared spectrograph. We combine these data, which span the 1.125-1.643 μm wavelength range, with broadband transit measurements made using Kepler/K2 (0.6-0.9 μm) and Spitzer/IRAC (4-5 μm). We find evidence for absorption by at least one of H2O, HCN, CO2, and CH4 (Bayes factor 7.4; 2.5σ significance), although the data precision does not allow us to unambiguously discriminate between these molecules. The transmission spectrum rules out cloud-free hydrogen-dominated atmospheres with metallicities ≤100 solar at &amp;gt;5.8σ confidence. In contrast, good agreement with the data is obtained for cloud-free models assuming metallicities &amp;gt;700 solar. However, for retrieval analyses that include the effect of clouds, a much broader range of metallicities (including subsolar) is consistent with the data, due to the degeneracy with cloud-top pressure....</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/8bg71322</guid>
      <pubDate>Tue, 2 Feb 2021 00:00:00 +0000</pubDate>
      <author>
        <name>Mikal-Evans, Thomas</name>
      </author>
      <author>
        <name>Crossfield, Ian JM</name>
      </author>
      <author>
        <name>Benneke, Björn</name>
      </author>
      <author>
        <name>Kreidberg, Laura</name>
      </author>
      <author>
        <name>Moses, Julie</name>
      </author>
      <author>
        <name>Morley, Caroline V</name>
      </author>
      <author>
        <name>Thorngren, Daniel</name>
      </author>
      <author>
        <name>Mollière, Paul</name>
      </author>
      <author>
        <name>Hardegree-Ullman, Kevin K</name>
      </author>
      <author>
        <name>Brewer, John</name>
      </author>
      <author>
        <name>Christiansen, Jessie L</name>
      </author>
      <author>
        <name>Ciardi, David R</name>
      </author>
      <author>
        <name>Dragomir, Diana</name>
      </author>
      <author>
        <name>Dressing, Courtney</name>
        <uri>https://orcid.org/0000-0001-8189-0233</uri>
      </author>
      <author>
        <name>Fortney, Jonathan J</name>
        <uri>https://orcid.org/0000-0002-9843-4354</uri>
      </author>
      <author>
        <name>Gorjian, Varoujan</name>
      </author>
      <author>
        <name>Greene, Thomas P</name>
      </author>
      <author>
        <name>Hirsch, Lea A</name>
      </author>
      <author>
        <name>Howard, Andrew W</name>
      </author>
      <author>
        <name>Howell, Steve B</name>
      </author>
      <author>
        <name>Isaacson, Howard</name>
        <uri>https://orcid.org/0000-0002-0531-1073</uri>
      </author>
      <author>
        <name>Kosiarek, Molly R</name>
      </author>
      <author>
        <name>Krick, Jessica</name>
      </author>
      <author>
        <name>Livingston, John H</name>
      </author>
      <author>
        <name>Lothringer, Joshua D</name>
      </author>
      <author>
        <name>Morales, Farisa Y</name>
      </author>
      <author>
        <name>Petigura, Erik A</name>
      </author>
      <author>
        <name>Schlieder, Joshua E</name>
      </author>
      <author>
        <name>Werner, Michael</name>
      </author>
    </item>
    <item>
      <title>Measuring the Hubble constant with a sample of kilonovae</title>
      <link>https://escholarship.org/uc/item/1wc7c1rt</link>
      <description>Kilonovae produced by the coalescence of compact binaries with at least one neutron star are promising standard sirens for an independent measurement of the Hubble constant (H0). Through their detection via follow-up of gravitational-wave (GW), short gamma-ray bursts (sGRBs) or optical surveys, a large sample of kilonovae (even without GW data) can be used for H0 contraints. Here, we show measurement of H0 using light curves associated with four sGRBs, assuming these are attributable to kilonovae, combined with GW170817. Including a systematic uncertainty on the models that is as large as the statistical ones, we find H0=73.8−5.8+6.3kms−1Mpc−1$${H}_{0}=73.{8}_{-5.8}^{+6.3}\ {\rm{km}}\ {{\rm{s}}}^{-1}\ {{\rm{Mpc}}}^{-1}$$ and H0=71.2−3.1+3.2kms−1Mpc−1$${H}_{0}=71.{2}_{-3.1}^{+3.2}\ {\rm{km}}\ {{\rm{s}}}^{-1}\ {{\rm{Mpc}}}^{-1}$$ for two different kilonova models that are consistent with the local and inverse-distance ladder measurements. For a given model, this measurement is about...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/1wc7c1rt</guid>
      <pubDate>Mon, 7 Sep 2020 00:00:00 +0000</pubDate>
      <author>
        <name>Coughlin, Michael W</name>
      </author>
      <author>
        <name>Antier, Sarah</name>
      </author>
      <author>
        <name>Dietrich, Tim</name>
      </author>
      <author>
        <name>Foley, Ryan J</name>
        <uri>https://orcid.org/0000-0002-2445-5275</uri>
      </author>
      <author>
        <name>Heinzel, Jack</name>
      </author>
      <author>
        <name>Bulla, Mattia</name>
      </author>
      <author>
        <name>Christensen, Nelson</name>
      </author>
      <author>
        <name>Coulter, David A</name>
      </author>
      <author>
        <name>Issa, Lina</name>
      </author>
      <author>
        <name>Khetan, Nandita</name>
      </author>
    </item>
    <item>
      <title>Saturn’s&amp;nbsp;Probable Interior: An Exploration of Saturn’s Potential Interior Density Structures</title>
      <link>https://escholarship.org/uc/item/0vn7g57f</link>
      <description>Saturn’s&amp;nbsp;Probable Interior: An Exploration of Saturn’s Potential Interior Density Structures</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/0vn7g57f</guid>
      <pubDate>Thu, 20 Aug 2020 00:00:00 +0000</pubDate>
      <author>
        <name>Movshovitz, Naor</name>
      </author>
      <author>
        <name>Fortney, Jonathan J</name>
      </author>
      <author>
        <name>Mankovich, Chris</name>
      </author>
      <author>
        <name>Thorngren, Daniel</name>
      </author>
      <author>
        <name>Helled, Ravit</name>
      </author>
    </item>
    <item>
      <title>The 16th Data Release of the Sloan Digital Sky Surveys: First Release from the APOGEE-2 Southern Survey and Full Release of eBOSS Spectra</title>
      <link>https://escholarship.org/uc/item/9j80t4m1</link>
      <description>This paper documents the 16th data release (DR16) from the Sloan Digital Sky Surveys (SDSS), the fourth and penultimate from the fourth phase (SDSS-IV). This is the first release of data from the Southern Hemisphere survey of the Apache Point Observatory Galactic Evolution Experiment 2 (APOGEE-2); new data from APOGEE-2 North are also included. DR16 is also notable as the final data release for the main cosmological program of the Extended Baryon Oscillation Spectroscopic Survey (eBOSS), and all raw and reduced spectra from that project are released here. DR16 also includes all the data from the Time Domain Spectroscopic Survey and new data from the SPectroscopic IDentification of ERosita Survey programs, both of which were co-observed on eBOSS plates. DR16 has no new data from the Mapping Nearby Galaxies at Apache Point Observatory (MaNGA) survey (or the MaNGA Stellar Library “MaStar”). We also preview future SDSS-V operations (due to start in 2020), and summarize plans for the...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/9j80t4m1</guid>
      <pubDate>Tue, 18 Aug 2020 00:00:00 +0000</pubDate>
      <author>
        <name>Ahumada, Romina</name>
      </author>
      <author>
        <name>Prieto, Carlos Allende</name>
      </author>
      <author>
        <name>Almeida, Andrés</name>
      </author>
      <author>
        <name>Anders, Friedrich</name>
      </author>
      <author>
        <name>Anderson, Scott F</name>
      </author>
      <author>
        <name>Andrews, Brett H</name>
      </author>
      <author>
        <name>Anguiano, Borja</name>
      </author>
      <author>
        <name>Arcodia, Riccardo</name>
      </author>
      <author>
        <name>Armengaud, Eric</name>
      </author>
      <author>
        <name>Aubert, Marie</name>
      </author>
      <author>
        <name>Avila, Santiago</name>
      </author>
      <author>
        <name>Avila-Reese, Vladimir</name>
      </author>
      <author>
        <name>Badenes, Carles</name>
      </author>
      <author>
        <name>Balland, Christophe</name>
      </author>
      <author>
        <name>Barger, Kat</name>
      </author>
      <author>
        <name>Barrera-Ballesteros, Jorge K</name>
      </author>
      <author>
        <name>Basu, Sarbani</name>
      </author>
      <author>
        <name>Bautista, Julian</name>
      </author>
      <author>
        <name>Beaton, Rachael L</name>
      </author>
      <author>
        <name>Beers, Timothy C</name>
      </author>
      <author>
        <name>Benavides, B Izamar T</name>
      </author>
      <author>
        <name>Bender, Chad F</name>
      </author>
      <author>
        <name>Bernardi, Mariangela</name>
      </author>
      <author>
        <name>Bershady, Matthew</name>
      </author>
      <author>
        <name>Beutler, Florian</name>
      </author>
      <author>
        <name>Bidin, Christian Moni</name>
      </author>
      <author>
        <name>Bird, Jonathan</name>
      </author>
      <author>
        <name>Bizyaev, Dmitry</name>
      </author>
      <author>
        <name>Blanc, Guillermo A</name>
      </author>
      <author>
        <name>Blanton, Michael R</name>
      </author>
      <author>
        <name>Boquien, Médéric</name>
      </author>
      <author>
        <name>Borissova, Jura</name>
      </author>
      <author>
        <name>Bovy, Jo</name>
      </author>
      <author>
        <name>Brandt, WN</name>
      </author>
      <author>
        <name>Brinkmann, Jonathan</name>
      </author>
      <author>
        <name>Brownstein, Joel R</name>
      </author>
      <author>
        <name>Bundy, Kevin</name>
      </author>
      <author>
        <name>Bureau, Martin</name>
      </author>
      <author>
        <name>Burgasser, Adam</name>
        <uri>https://orcid.org/0000-0002-6523-9536</uri>
      </author>
      <author>
        <name>Burtin, Etienne</name>
      </author>
      <author>
        <name>Cano-Díaz, Mariana</name>
      </author>
      <author>
        <name>Capasso, Raffaella</name>
      </author>
      <author>
        <name>Cappellari, Michele</name>
      </author>
      <author>
        <name>Carrera, Ricardo</name>
      </author>
      <author>
        <name>Chabanier, Solène</name>
        <uri>https://orcid.org/0000-0002-5692-5243</uri>
      </author>
      <author>
        <name>Chaplin, William</name>
      </author>
      <author>
        <name>Chapman, Michael</name>
      </author>
      <author>
        <name>Cherinka, Brian</name>
      </author>
      <author>
        <name>Chiappini, Cristina</name>
      </author>
      <author>
        <name>Choi, Peter Doohyun</name>
      </author>
      <author>
        <name>Chojnowski, S Drew</name>
      </author>
      <author>
        <name>Chung, Haeun</name>
      </author>
      <author>
        <name>Clerc, Nicolas</name>
      </author>
      <author>
        <name>Coffey, Damien</name>
      </author>
      <author>
        <name>Comerford, Julia M</name>
      </author>
      <author>
        <name>Comparat, Johan</name>
      </author>
      <author>
        <name>da Costa, Luiz</name>
      </author>
      <author>
        <name>Cousinou, Marie-Claude</name>
      </author>
      <author>
        <name>Covey, Kevin</name>
      </author>
      <author>
        <name>Crane, Jeffrey D</name>
      </author>
      <author>
        <name>Cunha, Katia</name>
      </author>
      <author>
        <name>da Silva Ilha, Gabriele</name>
      </author>
      <author>
        <name>Dai, Yu Sophia</name>
      </author>
      <author>
        <name>Damsted, Sanna B</name>
      </author>
      <author>
        <name>Darling, Jeremy</name>
      </author>
      <author>
        <name>Davidson, James W</name>
      </author>
      <author>
        <name>Davies, Roger</name>
      </author>
      <author>
        <name>Dawson, Kyle</name>
      </author>
      <author>
        <name>De, Nikhil</name>
      </author>
      <author>
        <name>de la Macorra, Axel</name>
      </author>
      <author>
        <name>De Lee, Nathan</name>
      </author>
      <author>
        <name>de Andrade Queiroz, Anna Bárbara</name>
      </author>
      <author>
        <name>Machado, Alice Deconto</name>
      </author>
      <author>
        <name>de la Torre, Sylvain</name>
      </author>
      <author>
        <name>Dell’Agli, Flavia</name>
      </author>
      <author>
        <name>du Mas des Bourboux, Hélion</name>
      </author>
      <author>
        <name>Diamond-Stanic, Aleksandar M</name>
      </author>
      <author>
        <name>Dillon, Sean</name>
      </author>
      <author>
        <name>Donor, John</name>
      </author>
      <author>
        <name>Drory, Niv</name>
      </author>
      <author>
        <name>Duckworth, Chris</name>
      </author>
      <author>
        <name>Dwelly, Tom</name>
      </author>
      <author>
        <name>Ebelke, Garrett</name>
      </author>
      <author>
        <name>Eftekharzadeh, Sarah</name>
      </author>
      <author>
        <name>Eigenbrot, Arthur Davis</name>
      </author>
      <author>
        <name>Elsworth, Yvonne P</name>
      </author>
      <author>
        <name>Eracleous, Mike</name>
      </author>
      <author>
        <name>Erfanianfar, Ghazaleh</name>
      </author>
      <author>
        <name>Escoffier, Stephanie</name>
      </author>
      <author>
        <name>Fan, Xiaohui</name>
      </author>
      <author>
        <name>Farr, Emily</name>
      </author>
      <author>
        <name>Fernández-Trincado, José G</name>
      </author>
      <author>
        <name>Feuillet, Diane</name>
      </author>
      <author>
        <name>Finoguenov, Alexis</name>
      </author>
      <author>
        <name>Fofie, Patricia</name>
      </author>
      <author>
        <name>Fraser-McKelvie, Amelia</name>
      </author>
      <author>
        <name>Frinchaboy, Peter M</name>
      </author>
      <author>
        <name>Fromenteau, Sebastien</name>
      </author>
      <author>
        <name>Fu, Hai</name>
      </author>
      <author>
        <name>Galbany, Lluís</name>
      </author>
    </item>
    <item>
      <title>ProtoDESI: First On-Sky Technology Demonstration for the Dark Energy Spectroscopic Instrument</title>
      <link>https://escholarship.org/uc/item/55n6t108</link>
      <description>The Dark Energy Spectroscopic Instrument (DESI) is under construction to measure the expansion history of the universe using the baryon acoustic oscillations technique. The spectra of 35 million galaxies and quasars over 14,000 square degrees will be measured during a 5-year survey. A new prime focus corrector for the Mayall telescope at Kitt Peak National Observatory will deliver light to 5,000 individually targeted fiber-fed robotic positioners. The fibers in turn feed ten broadband multi-object spectrographs. We describe the ProtoDESI experiment, that was installed and commissioned on the 4-m Mayall telescope from 2016 August 14 to September 30. ProtoDESI was an on-sky technology demonstration with the goal to reduce technical risks associated with aligning optical fibers with targets using robotic fiber positioners and maintaining the stability required to operate DESI. The ProtoDESI prime focus instrument, consisting of three fiber positioners, illuminated fiducials, and...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/55n6t108</guid>
      <pubDate>Tue, 18 Aug 2020 00:00:00 +0000</pubDate>
      <author>
        <name>Fagrelius, Parker</name>
      </author>
      <author>
        <name>Abareshi, Behzad</name>
      </author>
      <author>
        <name>Allen, Lori</name>
      </author>
      <author>
        <name>Ballester, Otger</name>
      </author>
      <author>
        <name>Baltay, Charles</name>
      </author>
      <author>
        <name>Besuner, Robert</name>
      </author>
      <author>
        <name>Buckley-Geer, Elizabeth</name>
      </author>
      <author>
        <name>Butler, Karen</name>
      </author>
      <author>
        <name>Cardiel, Laia</name>
      </author>
      <author>
        <name>Dey, Arjun</name>
      </author>
      <author>
        <name>Duan, Yutong</name>
      </author>
      <author>
        <name>Elliott, Ann</name>
      </author>
      <author>
        <name>Emmet, William</name>
      </author>
      <author>
        <name>Gershkovich, Irena</name>
      </author>
      <author>
        <name>Honscheid, Klaus</name>
      </author>
      <author>
        <name>Illa, Jose M</name>
      </author>
      <author>
        <name>Jimenez, Jorge</name>
      </author>
      <author>
        <name>Joyce, Richard</name>
      </author>
      <author>
        <name>Karcher, Armin</name>
      </author>
      <author>
        <name>Kent, Stephen</name>
      </author>
      <author>
        <name>Lambert, Andrew</name>
        <uri>https://orcid.org/0009-0003-5658-2601</uri>
      </author>
      <author>
        <name>Lampton, Michael</name>
      </author>
      <author>
        <name>Levi, Michael</name>
        <uri>https://orcid.org/0000-0003-1887-1018</uri>
      </author>
      <author>
        <name>Manser, Christopher</name>
      </author>
      <author>
        <name>Marshall, Robert</name>
      </author>
      <author>
        <name>Martini, Paul</name>
      </author>
      <author>
        <name>Paat, Anthony</name>
      </author>
      <author>
        <name>Probst, Ronald</name>
      </author>
      <author>
        <name>Rabinowitz, David</name>
      </author>
      <author>
        <name>Reil, Kevin</name>
      </author>
      <author>
        <name>Robertson, Amy</name>
      </author>
      <author>
        <name>Rockosi, Connie</name>
      </author>
      <author>
        <name>Schlegel, David</name>
        <uri>https://orcid.org/0000-0002-5042-5088</uri>
      </author>
      <author>
        <name>Schubnell, Michael</name>
      </author>
      <author>
        <name>Serrano, Santiago</name>
      </author>
      <author>
        <name>Silber, Joseph</name>
        <uri>https://orcid.org/0000-0002-3461-0320</uri>
      </author>
      <author>
        <name>Soto, Christian</name>
      </author>
      <author>
        <name>Sprayberry, David</name>
      </author>
      <author>
        <name>Summers, David</name>
      </author>
      <author>
        <name>Tarlé, Greg</name>
      </author>
      <author>
        <name>Weaver, Benjamin A</name>
      </author>
    </item>
    <item>
      <title>HALO7D II: The Halo Velocity Ellipsoid and Velocity Anisotropy with Distant Main-sequence Stars</title>
      <link>https://escholarship.org/uc/item/7kn6z3zw</link>
      <description>The Halo Assembly in Lambda Cold Dark Matter: Observations in 7 Dimensions (HALO7D) data set consists of Keck II/DEIMOS spectroscopy and Hubble Space Telescope–measured proper motions of Milky Way halo main-sequence turnoff stars in the CANDELS fields. In this paper, the second in the HALO7D series, we present the proper motions for the HALO7D sample. We discuss our measurement methodology, which makes use of a Bayesian mixture modeling approach for creating the stationary reference frame of distant galaxies. Using the 3D kinematic HALO7D sample, we estimate the parameters of the halo velocity ellipsoid, , and the velocity anisotropy β. Using the full HALO7D sample, we find at kpc. We also estimate the ellipsoid parameters for our sample split into three apparent magnitude bins; the posterior medians for these estimates of β are consistent with one another. Finally, we estimate β in each of the individual HALO7D fields. We find that the velocity anisotropy β can vary from field-to...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/7kn6z3zw</guid>
      <pubDate>Wed, 10 Jun 2020 00:00:00 +0000</pubDate>
      <author>
        <name>Cunningham, Emily C</name>
      </author>
      <author>
        <name>Deason, Alis J</name>
      </author>
      <author>
        <name>Sanderson, Robyn E</name>
      </author>
      <author>
        <name>Sohn, Sangmo Tony</name>
      </author>
      <author>
        <name>Anderson, Jay</name>
      </author>
      <author>
        <name>Guhathakurta, Puragra</name>
      </author>
      <author>
        <name>Rockosi, Constance M</name>
      </author>
      <author>
        <name>van der Marel, Roeland P</name>
      </author>
      <author>
        <name>Loebman, Sarah R</name>
      </author>
      <author>
        <name>Wetzel, Andrew</name>
        <uri>https://orcid.org/0000-0003-0603-8942</uri>
      </author>
    </item>
    <item>
      <title>Saturn’s Probable Interior: An Exploration of Saturn’s Potential Interior Density Structures</title>
      <link>https://escholarship.org/uc/item/6f8365cc</link>
      <description>Saturn’s Probable Interior: An Exploration of Saturn’s Potential Interior Density Structures</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/6f8365cc</guid>
      <pubDate>Tue, 2 Jun 2020 00:00:00 +0000</pubDate>
      <author>
        <name>Movshovitz, Naor</name>
      </author>
      <author>
        <name>Fortney, Jonathan J</name>
      </author>
      <author>
        <name>Mankovich, Chris</name>
      </author>
      <author>
        <name>Thorngren, Daniel</name>
      </author>
      <author>
        <name>Helled, Ravit</name>
      </author>
    </item>
    <item>
      <title>The photoheating of the intergalactic medium in synthesis models of the UV background</title>
      <link>https://escholarship.org/uc/item/4q1641x6</link>
      <description>We compare cosmological hydrodynamical simulations combined with the homogeneous metagalactic UV background (UVB) of Haardt &amp;amp; Madau (hereafter HM2012) to observations of the Lyman α forest that are sensitive to the thermal and ionization state of the intergalactic medium (IGM). The transition from optically thick to thin photoheating predicted by the simple one-zone, radiative transfer model implemented by HM2012 predicts a thermal history that is in remarkably good agreement with the observed rise of the IGM temperature at z ∼ 3 if we account for the expected evolution of the volume filling factor of He iii. Our simulations indicate that there may be, however, some tension between the observed peak in the temperature evolution and the rather slow evolution of the He ii opacities suggested by recent Hubble Space Telescope/Cosmic Origins Spectrograph measurements. The HM2012 UVB also underpredicts the metagalactic hydrogen photoionization rate required by our simulations to...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/4q1641x6</guid>
      <pubDate>Wed, 20 May 2020 00:00:00 +0000</pubDate>
      <author>
        <name>Puchwein, Ewald</name>
      </author>
      <author>
        <name>Bolton, James S</name>
      </author>
      <author>
        <name>Haehnelt, Martin G</name>
      </author>
      <author>
        <name>Madau, Piero</name>
        <uri>https://orcid.org/0000-0002-6336-3293</uri>
      </author>
      <author>
        <name>Becker, George D</name>
      </author>
      <author>
        <name>Haardt, Francesco</name>
      </author>
    </item>
    <item>
      <title>Reverse Shock Emission Revealed in Early Photometry in the Candidate Short GRB 180418A</title>
      <link>https://escholarship.org/uc/item/1g07f9c8</link>
      <description>We present observations of the possible short GRB 180418A in γ-rays, X-rays, and in the optical. Early optical photometry with the TAROT and RATIR instruments shows a bright peak (≈14.2 AB mag) between T + 28 and T + 90 s that we interpret as the signature of a reverse shock. Later observations can be modeled by a standard forward shock model and show no evidence of a jet break, allowing us to constrain the jet collimation to θj &amp;gt; 7°. Using deep late-time optical observations, we place an upper limit of r &amp;gt; 24 AB mag on any underlying host galaxy. The detection of the afterglow in the Swift UV filters constrains the GRB redshift to z &amp;lt; 1.3 and places an upper bound on the γ-ray isotropic equivalent energy Eγ,iso &amp;lt; 3 × 1051 erg. The properties of this GRB (e.g., duration, hardness ratio, energy, and environment) lie at the intersection between short and long bursts, and we cannot conclusively identify its type. We estimate that the probability that it is drawn from...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/1g07f9c8</guid>
      <pubDate>Fri, 24 Apr 2020 00:00:00 +0000</pubDate>
      <author>
        <name>Becerra, RL</name>
      </author>
      <author>
        <name>Dichiara, S</name>
      </author>
      <author>
        <name>Watson, AM</name>
      </author>
      <author>
        <name>Troja, E</name>
      </author>
      <author>
        <name>Fraija, N</name>
      </author>
      <author>
        <name>Klotz, A</name>
      </author>
      <author>
        <name>Butler, NR</name>
      </author>
      <author>
        <name>Lee, WH</name>
      </author>
      <author>
        <name>Veres, P</name>
      </author>
      <author>
        <name>Turpin, D</name>
      </author>
      <author>
        <name>Bloom, JS</name>
      </author>
      <author>
        <name>Boer, M</name>
      </author>
      <author>
        <name>González, JJ</name>
      </author>
      <author>
        <name>Kutyrev, AS</name>
      </author>
      <author>
        <name>Prochaska, JX</name>
      </author>
      <author>
        <name>Ramirez-Ruiz, E</name>
        <uri>https://orcid.org/0000-0003-2558-3102</uri>
      </author>
      <author>
        <name>Richer, MG</name>
      </author>
    </item>
    <item>
      <title>First cosmology results using type Ia supernovae from the Dark Energy Survey: the effect of host galaxy properties on supernova luminosity</title>
      <link>https://escholarship.org/uc/item/8p62m7fn</link>
      <description>ABSTRACT
                  We present improved photometric measurements for the host galaxies of 206 spectroscopically confirmed type Ia supernovae discovered by the Dark Energy Survey Supernova Program (DES-SN) and used in the first DES-SN cosmological analysis. For the DES-SN sample, when considering a 5D (z, x1, c, α, β) bias correction, we find evidence of a Hubble residual ‘mass step’, where SNe Ia in high-mass galaxies (&amp;gt;1010M⊙) are intrinsically more luminous (after correction) than their low-mass counterparts by $\gamma =0.040\pm 0.019$ mag. This value is larger by 0.031&amp;nbsp;mag than the value found in the first DES-SN cosmological analysis. This difference is due to a combination of updated photometric measurements and improved star formation histories and is not from host-galaxy misidentification. When using a 1D (redshift-only) bias correction the inferred mass step is larger, with $\gamma =0.066\pm 0.020$ mag. The 1D−5D γ difference for DES-SN is $0.026\pm 0.009$...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/8p62m7fn</guid>
      <pubDate>Tue, 17 Mar 2020 00:00:00 +0000</pubDate>
      <author>
        <name>Smith, M</name>
      </author>
      <author>
        <name>Sullivan, M</name>
      </author>
      <author>
        <name>Wiseman, P</name>
      </author>
      <author>
        <name>Kessler, R</name>
      </author>
      <author>
        <name>Scolnic, D</name>
      </author>
      <author>
        <name>Brout, D</name>
      </author>
      <author>
        <name>D’Andrea, CB</name>
      </author>
      <author>
        <name>Davis, TM</name>
      </author>
      <author>
        <name>Foley, RJ</name>
        <uri>https://orcid.org/0000-0002-2445-5275</uri>
      </author>
      <author>
        <name>Frohmaier, C</name>
      </author>
      <author>
        <name>Galbany, L</name>
      </author>
      <author>
        <name>Gupta, RR</name>
      </author>
      <author>
        <name>Gutiérrez, CP</name>
      </author>
      <author>
        <name>Hinton, SR</name>
      </author>
      <author>
        <name>Kelsey, L</name>
      </author>
      <author>
        <name>Lidman, C</name>
      </author>
      <author>
        <name>Macaulay, E</name>
      </author>
      <author>
        <name>Möller, A</name>
      </author>
      <author>
        <name>Nichol, RC</name>
      </author>
      <author>
        <name>Nugent, P</name>
        <uri>https://orcid.org/0000-0002-3389-0586</uri>
      </author>
      <author>
        <name>Palmese, A</name>
      </author>
      <author>
        <name>Pursiainen, M</name>
      </author>
      <author>
        <name>Sako, M</name>
      </author>
      <author>
        <name>Swann, E</name>
      </author>
      <author>
        <name>Thomas, RC</name>
      </author>
      <author>
        <name>Tucker, BE</name>
      </author>
      <author>
        <name>Vincenzi, M</name>
      </author>
      <author>
        <name>Carollo, D</name>
      </author>
      <author>
        <name>Lewis, GF</name>
      </author>
      <author>
        <name>Sommer, NE</name>
      </author>
      <author>
        <name>Abbott, TMC</name>
      </author>
      <author>
        <name>Aguena, M</name>
      </author>
      <author>
        <name>Allam, S</name>
      </author>
      <author>
        <name>Avila, S</name>
      </author>
      <author>
        <name>Bertin, E</name>
      </author>
      <author>
        <name>Bhargava, S</name>
      </author>
      <author>
        <name>Brooks, D</name>
      </author>
      <author>
        <name>Buckley-Geer, E</name>
      </author>
      <author>
        <name>Burke, DL</name>
      </author>
      <author>
        <name>Rosell, A Carnero</name>
      </author>
      <author>
        <name>Kind, M Carrasco</name>
      </author>
      <author>
        <name>Costanzi, M</name>
      </author>
      <author>
        <name>da Costa, LN</name>
      </author>
      <author>
        <name>De Vicente, J</name>
      </author>
      <author>
        <name>Desai, S</name>
      </author>
      <author>
        <name>Diehl, HT</name>
      </author>
      <author>
        <name>Doel, P</name>
      </author>
      <author>
        <name>Eifler, TF</name>
      </author>
      <author>
        <name>Everett, S</name>
      </author>
      <author>
        <name>Flaugher, B</name>
      </author>
      <author>
        <name>Fosalba, P</name>
      </author>
      <author>
        <name>Frieman, J</name>
      </author>
      <author>
        <name>García-Bellido, J</name>
      </author>
      <author>
        <name>Gaztanaga, E</name>
      </author>
      <author>
        <name>Glazebrook, K</name>
      </author>
      <author>
        <name>Gruen, D</name>
      </author>
      <author>
        <name>Gruendl, RA</name>
      </author>
      <author>
        <name>Gschwend, J</name>
      </author>
      <author>
        <name>Gutierrez, G</name>
      </author>
      <author>
        <name>Hartley, WG</name>
      </author>
      <author>
        <name>Hollowood, DL</name>
      </author>
      <author>
        <name>Honscheid, K</name>
      </author>
      <author>
        <name>James, DJ</name>
      </author>
      <author>
        <name>Krause, E</name>
      </author>
      <author>
        <name>Kuehn, K</name>
      </author>
      <author>
        <name>Kuropatkin, N</name>
      </author>
      <author>
        <name>Lima, M</name>
      </author>
      <author>
        <name>MacCrann, N</name>
      </author>
      <author>
        <name>Maia, MAG</name>
      </author>
      <author>
        <name>Marshall, JL</name>
      </author>
      <author>
        <name>Martini, P</name>
      </author>
      <author>
        <name>Melchior, P</name>
      </author>
      <author>
        <name>Menanteau, F</name>
      </author>
      <author>
        <name>Miquel, R</name>
      </author>
      <author>
        <name>Paz-Chinchón, F</name>
      </author>
      <author>
        <name>Plazas, AA</name>
      </author>
      <author>
        <name>Romer, AK</name>
      </author>
      <author>
        <name>Roodman, A</name>
      </author>
      <author>
        <name>Rykoff, ES</name>
      </author>
      <author>
        <name>Sanchez, E</name>
      </author>
      <author>
        <name>Scarpine, V</name>
      </author>
      <author>
        <name>Schubnell, M</name>
      </author>
      <author>
        <name>Serrano, S</name>
      </author>
      <author>
        <name>Sevilla-Noarbe, I</name>
      </author>
      <author>
        <name>Suchyta, E</name>
      </author>
      <author>
        <name>Swanson, MEC</name>
      </author>
      <author>
        <name>Tarle, G</name>
      </author>
      <author>
        <name>Thomas, D</name>
      </author>
      <author>
        <name>Tucker, DL</name>
      </author>
      <author>
        <name>Varga, TN</name>
      </author>
      <author>
        <name>Walker, AR</name>
      </author>
    </item>
    <item>
      <title>DES16C3cje: A low-luminosity, long-lived supernova</title>
      <link>https://escholarship.org/uc/item/2m30b199</link>
      <description>ABSTRACT
                  We present DES16C3cje, a low-luminosity, long-lived type II supernova (SN&amp;nbsp;II) at redshift 0.0618, detected by the Dark Energy Survey (DES). DES16C3cje is a unique SN. The spectra are characterized by extremely narrow photospheric lines corresponding to very low expansion velocities of ≲1500 km s−1, and the light curve shows an initial peak that fades after 50 d before slowly rebrightening over a further 100 d to reach an absolute brightness of Mr&amp;nbsp;∼ −15.5 mag. The decline rate of the late-time light curve is then slower than that expected from the powering by radioactive decay of 56Co, but is comparable to that expected from accretion power. Comparing the bolometric light curve with hydrodynamical models, we find that DES16C3cje can be explained by either (i) a low explosion energy (0.11 foe) and relatively large 56Ni production of 0.075 M⊙ from an&amp;nbsp;∼15 M⊙ red supergiant progenitor typical of other SNe&amp;nbsp;II, or (ii) a relatively compact...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/2m30b199</guid>
      <pubDate>Tue, 17 Mar 2020 00:00:00 +0000</pubDate>
      <author>
        <name>Gutiérrez, CP</name>
      </author>
      <author>
        <name>Sullivan, M</name>
      </author>
      <author>
        <name>Martinez, L</name>
      </author>
      <author>
        <name>Bersten, MC</name>
      </author>
      <author>
        <name>Inserra, C</name>
      </author>
      <author>
        <name>Smith, M</name>
      </author>
      <author>
        <name>Anderson, JP</name>
      </author>
      <author>
        <name>Pan, Y-C</name>
      </author>
      <author>
        <name>Pastorello, A</name>
      </author>
      <author>
        <name>Galbany, L</name>
      </author>
      <author>
        <name>Nugent, P</name>
        <uri>https://orcid.org/0000-0002-3389-0586</uri>
      </author>
      <author>
        <name>Angus, CR</name>
      </author>
      <author>
        <name>Barbarino, C</name>
      </author>
      <author>
        <name>Carollo, D</name>
      </author>
      <author>
        <name>Chen, T-W</name>
      </author>
      <author>
        <name>Davis, TM</name>
      </author>
      <author>
        <name>Della Valle, M</name>
      </author>
      <author>
        <name>Foley, RJ</name>
        <uri>https://orcid.org/0000-0002-2445-5275</uri>
      </author>
      <author>
        <name>Fraser, M</name>
      </author>
      <author>
        <name>Frohmaier, C</name>
      </author>
      <author>
        <name>González-Gaitán, S</name>
      </author>
      <author>
        <name>Gromadzki, M</name>
      </author>
      <author>
        <name>Kankare, E</name>
      </author>
      <author>
        <name>Kokotanekova, R</name>
      </author>
      <author>
        <name>Kollmeier, J</name>
      </author>
      <author>
        <name>Lewis, GF</name>
      </author>
      <author>
        <name>Magee, MR</name>
      </author>
      <author>
        <name>Maguire, K</name>
      </author>
      <author>
        <name>Möller, A</name>
      </author>
      <author>
        <name>Morrell, N</name>
      </author>
      <author>
        <name>Nicholl, M</name>
      </author>
      <author>
        <name>Pursiainen, M</name>
      </author>
      <author>
        <name>Sollerman, J</name>
      </author>
      <author>
        <name>Sommer, NE</name>
      </author>
      <author>
        <name>Swann, E</name>
      </author>
      <author>
        <name>Tucker, BE</name>
      </author>
      <author>
        <name>Wiseman, P</name>
      </author>
      <author>
        <name>Aguena, M</name>
      </author>
      <author>
        <name>Allam, S</name>
      </author>
      <author>
        <name>Avila, S</name>
      </author>
      <author>
        <name>Bertin, E</name>
      </author>
      <author>
        <name>Brooks, D</name>
      </author>
      <author>
        <name>Buckley-Geer, E</name>
      </author>
      <author>
        <name>Burke, DL</name>
      </author>
      <author>
        <name>Rosell, A Carnero</name>
      </author>
      <author>
        <name>Kind, M Carrasco</name>
      </author>
      <author>
        <name>Carretero, J</name>
      </author>
      <author>
        <name>Costanzi, M</name>
      </author>
      <author>
        <name>da Costa, LN</name>
      </author>
      <author>
        <name>De Vicente, J</name>
      </author>
      <author>
        <name>Desai, S</name>
      </author>
      <author>
        <name>Diehl, HT</name>
      </author>
      <author>
        <name>Doel, P</name>
      </author>
      <author>
        <name>Eifler, TF</name>
      </author>
      <author>
        <name>Flaugher, B</name>
      </author>
      <author>
        <name>Fosalba, P</name>
      </author>
      <author>
        <name>Frieman, J</name>
      </author>
      <author>
        <name>García-Bellido, J</name>
      </author>
      <author>
        <name>Gerdes, DW</name>
      </author>
      <author>
        <name>Gruen, D</name>
      </author>
      <author>
        <name>Gruendl, RA</name>
      </author>
      <author>
        <name>Gschwend, J</name>
      </author>
      <author>
        <name>Gutierrez, G</name>
      </author>
      <author>
        <name>Hinton, SR</name>
      </author>
      <author>
        <name>Hollowood, DL</name>
      </author>
      <author>
        <name>Honscheid, K</name>
      </author>
      <author>
        <name>James, DJ</name>
      </author>
      <author>
        <name>Kuehn, K</name>
      </author>
      <author>
        <name>Kuropatkin, N</name>
      </author>
      <author>
        <name>Lahav, O</name>
      </author>
      <author>
        <name>Lima, M</name>
      </author>
      <author>
        <name>Maia, MAG</name>
      </author>
      <author>
        <name>March, M</name>
      </author>
      <author>
        <name>Menanteau, F</name>
      </author>
      <author>
        <name>Miquel, R</name>
      </author>
      <author>
        <name>Morganson, E</name>
      </author>
      <author>
        <name>Palmese, A</name>
      </author>
      <author>
        <name>Paz-Chinchón, F</name>
      </author>
      <author>
        <name>Plazas, AA</name>
      </author>
      <author>
        <name>Sako, M</name>
      </author>
      <author>
        <name>Sanchez, E</name>
      </author>
      <author>
        <name>Scarpine, V</name>
      </author>
      <author>
        <name>Schubnell, M</name>
      </author>
      <author>
        <name>Serrano, S</name>
      </author>
      <author>
        <name>Sevilla-Noarbe, I</name>
      </author>
      <author>
        <name>Soares-Santos, M</name>
      </author>
      <author>
        <name>Suchyta, E</name>
      </author>
      <author>
        <name>Swanson, MEC</name>
      </author>
      <author>
        <name>Tarle, G</name>
      </author>
      <author>
        <name>Thomas, D</name>
      </author>
      <author>
        <name>Varga, TN</name>
      </author>
      <author>
        <name>Walker, AR</name>
      </author>
      <author>
        <name>Wilkinson, R</name>
      </author>
    </item>
    <item>
      <title>GRB 180620A: Evidence for Late-time Energy Injection</title>
      <link>https://escholarship.org/uc/item/22f589zr</link>
      <description>The early optical emission of gamma-ray bursts (GRBs) gives an opportunity to understand the central engine and first stages of these events. About 30% of GRBs present flares whose origin is still a subject of discussion. We present optical photometry of GRB 180620A with the COATLI telescope and RATIR instrument. COATLI started to observe from the end of prompt emission at T + 39.3 s and RATIR from T + 121.4 s. We supplement the optical data with the X-ray light curve from Swift/XRT. We observe an optical flare from T + 110 s to T + 550 s, with a temporal index decay αO,decay = 1.32 ± 0.01, and Δt/t = 1.63, which we interpret as the signature of a reverse shock component. After the initial normal decay the light curves show a long plateau from T + 500 s to T + 7800 s in both X-rays and the optical before decaying again after an achromatic jet break at T + 7800 s. Fluctuations are seen during the plateau phase in the optical. Adding to the complexity of GRB afterglows, the plateau...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/22f589zr</guid>
      <pubDate>Tue, 3 Mar 2020 00:00:00 +0000</pubDate>
      <author>
        <name>Becerra, RL</name>
      </author>
      <author>
        <name>De Colle, F</name>
      </author>
      <author>
        <name>Watson, AM</name>
      </author>
      <author>
        <name>Fraija, N</name>
      </author>
      <author>
        <name>Butler, NR</name>
      </author>
      <author>
        <name>Lee, WH</name>
      </author>
      <author>
        <name>Román-Zúñiga, CG</name>
      </author>
      <author>
        <name>Bloom, JS</name>
      </author>
      <author>
        <name>González, JJ</name>
      </author>
      <author>
        <name>Kutyrev, AS</name>
      </author>
      <author>
        <name>Prochaska, JX</name>
      </author>
      <author>
        <name>Ramirez-Ruiz, E</name>
        <uri>https://orcid.org/0000-0003-2558-3102</uri>
      </author>
      <author>
        <name>Richer, MG</name>
      </author>
      <author>
        <name>Troja, E</name>
      </author>
    </item>
    <item>
      <title>An Ultra Deep Field survey with WFIRST</title>
      <link>https://escholarship.org/uc/item/8mr8902f</link>
      <description>Studying the formation and evolution of galaxies at the earliest cosmic
times, and their role in reionization, requires the deepest imaging possible.
Ultra-deep surveys like the HUDF and HFF have pushed to mag \mAB$\,\sim\,$30,
revealing galaxies at the faint end of the LF to $z$$\,\sim\,$9$\,-\,$11 and
constraining their role in reionization. However, a key limitation of these
fields is their size, only a few arcminutes (less than a Mpc at these
redshifts), too small to probe large-scale environments or clustering
properties of these galaxies, crucial for advancing our understanding of
reionization. Achieving HUDF-quality depth over areas $\sim$100 times larger
becomes possible with a mission like the Wide Field Infrared Survey Telescope
(WFIRST), a 2.4-m telescope with similar optical properties to HST, with a
field of view of $\sim$1000 arcmin$^2$, $\sim$100$\times$ the area of the
HST/ACS HUDF.
  This whitepaper motivates an Ultra-Deep Field survey with WFIRST, covering
$\sim$100$\,-\,$300$\times$...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/8mr8902f</guid>
      <pubDate>Mon, 2 Dec 2019 00:00:00 +0000</pubDate>
      <author>
        <name>Koekemoer, Anton M</name>
      </author>
      <author>
        <name>Foley, RJ</name>
        <uri>https://orcid.org/0000-0002-2445-5275</uri>
      </author>
      <author>
        <name>Spergel, DN</name>
      </author>
      <author>
        <name>Bagley, M</name>
      </author>
      <author>
        <name>Bezanson, R</name>
      </author>
      <author>
        <name>Bianco, FB</name>
      </author>
      <author>
        <name>Bouwens, R</name>
      </author>
      <author>
        <name>Bradley, L</name>
      </author>
      <author>
        <name>Brammer, G</name>
      </author>
      <author>
        <name>Capak, P</name>
      </author>
      <author>
        <name>Davidzon, I</name>
      </author>
      <author>
        <name>Rosa, G De</name>
      </author>
      <author>
        <name>Dickinson, ME</name>
      </author>
      <author>
        <name>Doré, O</name>
      </author>
      <author>
        <name>Dunlop, JS</name>
      </author>
      <author>
        <name>Ellis, RS</name>
      </author>
      <author>
        <name>Fan, X</name>
      </author>
      <author>
        <name>Fazio, GG</name>
      </author>
      <author>
        <name>Ferguson, HC</name>
      </author>
      <author>
        <name>Filippenko, AV</name>
      </author>
      <author>
        <name>Finkelstein, S</name>
      </author>
      <author>
        <name>Frye, B</name>
      </author>
      <author>
        <name>Gawiser, E</name>
      </author>
      <author>
        <name>Grogin, NA</name>
      </author>
      <author>
        <name>Hathi, NP</name>
      </author>
      <author>
        <name>Hirata, CM</name>
      </author>
      <author>
        <name>Hounsell, R</name>
      </author>
      <author>
        <name>Illingworth, GD</name>
      </author>
      <author>
        <name>Jansen, RA</name>
      </author>
      <author>
        <name>Jauzac, M</name>
      </author>
      <author>
        <name>Jha, SW</name>
      </author>
      <author>
        <name>Kartaltepe, JS</name>
      </author>
      <author>
        <name>Kim, AG</name>
        <uri>https://orcid.org/0000-0001-6315-8743</uri>
      </author>
      <author>
        <name>Kelly, P</name>
      </author>
      <author>
        <name>Kruk, JW</name>
      </author>
      <author>
        <name>Larson, R</name>
      </author>
      <author>
        <name>Lotz, J</name>
      </author>
      <author>
        <name>Lucas, R</name>
      </author>
      <author>
        <name>Malhotra, S</name>
      </author>
      <author>
        <name>Mandel, K</name>
      </author>
      <author>
        <name>Margutti, R</name>
        <uri>https://orcid.org/0000-0003-4768-7586</uri>
      </author>
      <author>
        <name>Marrone, D</name>
      </author>
      <author>
        <name>McLure, RJ</name>
      </author>
      <author>
        <name>McQuinn, K</name>
      </author>
      <author>
        <name>Melchior, P</name>
      </author>
      <author>
        <name>Mobasher, B</name>
      </author>
      <author>
        <name>Mould, JR</name>
      </author>
      <author>
        <name>Moustakas, L</name>
      </author>
      <author>
        <name>Newman, JA</name>
      </author>
      <author>
        <name>Papovich, C</name>
      </author>
      <author>
        <name>Peeples, MS</name>
      </author>
      <author>
        <name>Perlmutter, S</name>
      </author>
      <author>
        <name>Pirzkal, N</name>
      </author>
      <author>
        <name>Rhoads, J</name>
      </author>
      <author>
        <name>Rhodes, J</name>
      </author>
      <author>
        <name>Robertson, B</name>
      </author>
      <author>
        <name>Rubin, D</name>
      </author>
      <author>
        <name>Ryan, R</name>
      </author>
      <author>
        <name>Scolnic, D</name>
      </author>
      <author>
        <name>Shapley, A</name>
      </author>
      <author>
        <name>Somerville, R</name>
      </author>
      <author>
        <name>Steinhardt, C</name>
      </author>
      <author>
        <name>Stiavelli, M</name>
      </author>
      <author>
        <name>Street, R</name>
      </author>
      <author>
        <name>Trenti, M</name>
      </author>
      <author>
        <name>Treu, T</name>
        <uri>https://orcid.org/0000-0002-8460-0390</uri>
      </author>
      <author>
        <name>Wang, L</name>
      </author>
      <author>
        <name>Wang, Y</name>
      </author>
      <author>
        <name>Whalen, D</name>
      </author>
      <author>
        <name>Windhorst, RA</name>
      </author>
      <author>
        <name>Wollack, EJ</name>
      </author>
      <author>
        <name>Yan, H</name>
      </author>
    </item>
    <item>
      <title>LSST Observing Strategy White Paper: LSST Observations of WFIRST Deep Fields</title>
      <link>https://escholarship.org/uc/item/1rs528tc</link>
      <description>The Wide-Field Infrared Survey Telescope (WFIRST) is expected to launch in
the mid-2020s. With its wide-field near-infrared (NIR) camera, it will survey
the sky to unprecedented detail. As part of normal operations and as the result
of multiple expected dedicated surveys, WFIRST will produce several relatively
wide-field (tens of square degrees) deep (limiting magnitude of 28 or fainter)
fields. In particular, a planned supernova survey is expected to image 3 deep
fields in the LSST footprint roughly every 5 days over 2 years. Stacking all
data, this survey will produce, over all WFIRST supernova fields in the LSST
footprint, ~12-25 deg^2 and ~5-15 deg^2 regions to depths of ~28 mag and ~29
mag, respectively. We suggest LSST undertake mini-surveys that will match the
WFIRST cadence and simultaneously observe the supernova survey fields during
the 2-year WFIRST supernova survey, achieving a stacked depth similar to that
of the WFIRST data. We also suggest additional observations...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/1rs528tc</guid>
      <pubDate>Mon, 2 Dec 2019 00:00:00 +0000</pubDate>
      <author>
        <name>Foley, RJ</name>
        <uri>https://orcid.org/0000-0002-2445-5275</uri>
      </author>
      <author>
        <name>Koekemoer, AM</name>
      </author>
      <author>
        <name>Spergel, DN</name>
      </author>
      <author>
        <name>Bianco, FB</name>
      </author>
      <author>
        <name>Capak, P</name>
      </author>
      <author>
        <name>Dai, L</name>
      </author>
      <author>
        <name>Dore, O</name>
      </author>
      <author>
        <name>Fazio, GG</name>
      </author>
      <author>
        <name>Ferguson, H</name>
      </author>
      <author>
        <name>Filippenko, AV</name>
      </author>
      <author>
        <name>Frye, B</name>
      </author>
      <author>
        <name>Galbany, L</name>
      </author>
      <author>
        <name>Gawiser, E</name>
      </author>
      <author>
        <name>Gronwall, C</name>
      </author>
      <author>
        <name>Hathi, NP</name>
      </author>
      <author>
        <name>Hirata, C</name>
      </author>
      <author>
        <name>Hounsell, R</name>
      </author>
      <author>
        <name>Jha, SW</name>
      </author>
      <author>
        <name>Kim, AG</name>
        <uri>https://orcid.org/0000-0001-6315-8743</uri>
      </author>
      <author>
        <name>Kelly, PL</name>
      </author>
      <author>
        <name>Kruk, JW</name>
      </author>
      <author>
        <name>Malhotra, S</name>
      </author>
      <author>
        <name>Mandel, KS</name>
      </author>
      <author>
        <name>Margutti, R</name>
      </author>
      <author>
        <name>Marrone, D</name>
      </author>
      <author>
        <name>McQuinn, KBW</name>
      </author>
      <author>
        <name>Melchior, P</name>
      </author>
      <author>
        <name>Moustakas, L</name>
      </author>
      <author>
        <name>Newman, JA</name>
      </author>
      <author>
        <name>Peek, JEG</name>
      </author>
      <author>
        <name>Perlmutter, S</name>
      </author>
      <author>
        <name>Rhodes, JD</name>
      </author>
      <author>
        <name>Robertson, B</name>
      </author>
      <author>
        <name>Rubin, D</name>
      </author>
      <author>
        <name>Scolnic, D</name>
      </author>
      <author>
        <name>Somerville, R</name>
      </author>
      <author>
        <name>Street, R</name>
      </author>
      <author>
        <name>Wang, Y</name>
      </author>
      <author>
        <name>Whalen, DJ</name>
      </author>
      <author>
        <name>Windhorst, RA</name>
      </author>
      <author>
        <name>Wollack, EJ</name>
      </author>
    </item>
    <item>
      <title>Deep ugrizY imaging and DEEP2/3 spectroscopy: a photometric redshift testbed for LSST and public release of data from the DEEP3 Galaxy Redshift Survey</title>
      <link>https://escholarship.org/uc/item/16x0j072</link>
      <description>ABSTRACT
                  We present catalogues of calibrated photometry and spectroscopic redshifts in the Extended Groth Strip, intended for studies of photometric redshifts (photo-z’s). The data includes ugriz photometry from Canada–France–Hawaii Telescope Legacy Survey (CFHTLS) and Y-band photometry from the Subaru Suprime camera, as well as spectroscopic redshifts from the DEEP2, DEEP3, and 3D-HST surveys. These catalogues incorporate corrections to produce effectively matched-aperture photometry across all bands, based upon object size information available in the catalogue and Moffat profile point spread function fits. We test this catalogue with a simple machine learning-based photometric redshift algorithm based upon Random Forest regression, and find that the corrected aperture photometry leads to significant improvement in photo-z accuracy compared to the original SExtractor catalogues from CFHTLS and Subaru. The deep ugrizY photometry and spectroscopic redshifts are...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/16x0j072</guid>
      <pubDate>Tue, 12 Nov 2019 00:00:00 +0000</pubDate>
      <author>
        <name>Zhou, Rongpu</name>
        <uri>https://orcid.org/0000-0001-5381-4372</uri>
      </author>
      <author>
        <name>Cooper, Michael C</name>
        <uri>https://orcid.org/0000-0003-1371-6019</uri>
      </author>
      <author>
        <name>Newman, Jeffrey A</name>
      </author>
      <author>
        <name>Ashby, Matthew LN</name>
      </author>
      <author>
        <name>Aird, James</name>
      </author>
      <author>
        <name>Conselice, Christopher J</name>
      </author>
      <author>
        <name>Davis, Marc</name>
      </author>
      <author>
        <name>Dutton, Aaron A</name>
      </author>
      <author>
        <name>Faber, SM</name>
      </author>
      <author>
        <name>Fang, Jerome J</name>
      </author>
      <author>
        <name>Fazio, GG</name>
      </author>
      <author>
        <name>Guhathakurta, Puragra</name>
      </author>
      <author>
        <name>Kocevski, Dale</name>
      </author>
      <author>
        <name>Koo, David C</name>
        <uri>https://orcid.org/0000-0003-3385-6799</uri>
      </author>
      <author>
        <name>Nandra, Kirpal</name>
      </author>
      <author>
        <name>Phillips, Andrew C</name>
      </author>
      <author>
        <name>Rosario, David J</name>
      </author>
      <author>
        <name>Schlafly, Edward F</name>
        <uri>https://orcid.org/0000-0002-3569-7421</uri>
      </author>
      <author>
        <name>Trump, Jonathan R</name>
      </author>
      <author>
        <name>Weiner, Benjamin</name>
      </author>
      <author>
        <name>Willmer, Christopher NA</name>
      </author>
      <author>
        <name>Yan, Renbin</name>
      </author>
    </item>
    <item>
      <title>The fast, luminous ultraviolet transient AT2018cow: extreme supernova, or disruption of a star by an intermediate-mass black hole?</title>
      <link>https://escholarship.org/uc/item/3db8r6g9</link>
      <description>Wide-field optical surveys have begun to uncover large samples of fast (trise ≲ 5 d), luminous (Mpeak &amp;lt; −18), blue transients. While commonly attributed to the breakout of a supernova shock into a dense wind, the great distances to the transients of this class found so far have hampered detailed investigation of their properties. We present photometry and spectroscopy from a comprehensive worldwide campaign to observe AT 2018cow (ATLAS 18qqn), the first fast-luminous optical transient to be found in real time at low redshift. Our first spectra (&amp;lt;2 days after discovery) are entirely featureless. A very broad absorption feature suggestive of near-relativistic velocities develops between 3 and 8 days, then disappears. Broad emission features of H and He develop after &amp;gt;10 days. The spectrum remains extremely hot throughout its evolution, and the photospheric radius contracts with time (receding below R &amp;lt; 1014 cm after 1 month). This behaviour does not match that of any...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/3db8r6g9</guid>
      <pubDate>Wed, 16 Oct 2019 00:00:00 +0000</pubDate>
      <author>
        <name>Perley, Daniel A</name>
      </author>
      <author>
        <name>Mazzali, Paolo A</name>
      </author>
      <author>
        <name>Yan, Lin</name>
      </author>
      <author>
        <name>Cenko, S Bradley</name>
      </author>
      <author>
        <name>Gezari, Suvi</name>
      </author>
      <author>
        <name>Taggart, Kirsty</name>
      </author>
      <author>
        <name>Blagorodnova, Nadia</name>
      </author>
      <author>
        <name>Fremling, Christoffer</name>
      </author>
      <author>
        <name>Mockler, Brenna</name>
      </author>
      <author>
        <name>Singh, Avinash</name>
      </author>
      <author>
        <name>Tominaga, Nozomu</name>
      </author>
      <author>
        <name>Tanaka, Masaomi</name>
      </author>
      <author>
        <name>Watson, Alan M</name>
      </author>
      <author>
        <name>Ahumada, Tomás</name>
      </author>
      <author>
        <name>Anupama, GC</name>
      </author>
      <author>
        <name>Ashall, Chris</name>
      </author>
      <author>
        <name>Becerra, Rosa L</name>
      </author>
      <author>
        <name>Bersier, David</name>
      </author>
      <author>
        <name>Bhalerao, Varun</name>
      </author>
      <author>
        <name>Bloom, Joshua S</name>
      </author>
      <author>
        <name>Butler, Nathaniel R</name>
      </author>
      <author>
        <name>Copperwheat, Chris</name>
      </author>
      <author>
        <name>Coughlin, Michael W</name>
      </author>
      <author>
        <name>De, Kishalay</name>
      </author>
      <author>
        <name>Drake, Andrew J</name>
      </author>
      <author>
        <name>Duev, Dmitry A</name>
      </author>
      <author>
        <name>Frederick, Sara</name>
      </author>
      <author>
        <name>González, J Jesús</name>
      </author>
      <author>
        <name>Goobar, Ariel</name>
      </author>
      <author>
        <name>Heida, Marianne</name>
      </author>
      <author>
        <name>Ho, Anna YQ</name>
      </author>
      <author>
        <name>Horst, John</name>
      </author>
      <author>
        <name>Hung, Tiara</name>
      </author>
      <author>
        <name>Itoh, Ryosuke</name>
      </author>
      <author>
        <name>Jencson, Jacob E</name>
      </author>
      <author>
        <name>Kasliwal, Mansi M</name>
      </author>
      <author>
        <name>Kawai, Nobuyuki</name>
      </author>
      <author>
        <name>Khanam, Tanazza</name>
      </author>
      <author>
        <name>Kulkarni, Shrinivas R</name>
      </author>
      <author>
        <name>Kumar, Brajesh</name>
      </author>
      <author>
        <name>Kumar, Harsh</name>
      </author>
      <author>
        <name>Kutyrev, Alexander S</name>
      </author>
      <author>
        <name>Lee, William H</name>
      </author>
      <author>
        <name>Maeda, Keiichi</name>
      </author>
      <author>
        <name>Mahabal, Ashish</name>
      </author>
      <author>
        <name>Murata, Katsuhiro L</name>
      </author>
      <author>
        <name>Neill, James D</name>
      </author>
      <author>
        <name>Ngeow, Chow-Choong</name>
      </author>
      <author>
        <name>Penprase, Bryan</name>
      </author>
      <author>
        <name>Pian, Elena</name>
      </author>
      <author>
        <name>Quimby, Robert</name>
      </author>
      <author>
        <name>Ramirez-Ruiz, Enrico</name>
        <uri>https://orcid.org/0000-0003-2558-3102</uri>
      </author>
      <author>
        <name>Richer, Michael G</name>
      </author>
      <author>
        <name>Román-Zúñiga, Carlos G</name>
      </author>
      <author>
        <name>Sahu, DK</name>
      </author>
      <author>
        <name>Srivastav, Shubham</name>
      </author>
      <author>
        <name>Socia, Quentin</name>
      </author>
      <author>
        <name>Sollerman, Jesper</name>
      </author>
      <author>
        <name>Tachibana, Yutaro</name>
      </author>
      <author>
        <name>Taddia, Francesco</name>
      </author>
      <author>
        <name>Tinyanont, Samaporn</name>
      </author>
      <author>
        <name>Troja, Eleonora</name>
      </author>
      <author>
        <name>Ward, Charlotte</name>
      </author>
      <author>
        <name>Wee, Jerrick</name>
      </author>
      <author>
        <name>Yu, Po-Chieh</name>
      </author>
    </item>
    <item>
      <title>Target of Opportunity Observations of Gravitational Wave Events with LSST</title>
      <link>https://escholarship.org/uc/item/2f18c097</link>
      <description>The discovery of the electromagnetic counterparts to the binary neutron star
merger GW170817 has opened the era of GW+EM multi-messenger astronomy.
Exploiting this breakthrough requires increasing samples to explore the
diversity of kilonova behaviour and provide more stringent constraints on the
Hubble constant, and tests of fundamental physics. LSST can play a key role in
this field in the 2020s, when the gravitational wave detector network is
expected to detect higher rates of merger events involving neutron stars
($\sim$10s per year) out to distances of several hundred Mpc. Here we propose
comprehensive target-of-opportunity (ToOs) strategies for follow-up of
gravitational-wave sources that will make LSST the premiere machine for
discovery and early characterization for neutron star mergers and other
gravitational-wave sources.</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/2f18c097</guid>
      <pubDate>Tue, 24 Sep 2019 00:00:00 +0000</pubDate>
      <author>
        <name>Margutti, R</name>
      </author>
      <author>
        <name>Cowperthwaite, P</name>
      </author>
      <author>
        <name>Doctor, Z</name>
      </author>
      <author>
        <name>Mortensen, K</name>
      </author>
      <author>
        <name>Pankow, CP</name>
      </author>
      <author>
        <name>Salafia, O</name>
      </author>
      <author>
        <name>Villar, VA</name>
      </author>
      <author>
        <name>Alexander, K</name>
      </author>
      <author>
        <name>Annis, J</name>
      </author>
      <author>
        <name>Andreoni, I</name>
      </author>
      <author>
        <name>Baldeschi, A</name>
      </author>
      <author>
        <name>Balmaverde, B</name>
      </author>
      <author>
        <name>Berger, E</name>
      </author>
      <author>
        <name>Bernardini, MG</name>
      </author>
      <author>
        <name>Berry, CPL</name>
      </author>
      <author>
        <name>Bianco, F</name>
      </author>
      <author>
        <name>Blanchard, PK</name>
      </author>
      <author>
        <name>Brocato, E</name>
      </author>
      <author>
        <name>Carnerero, MI</name>
      </author>
      <author>
        <name>Cartier, R</name>
      </author>
      <author>
        <name>Cenko, SB</name>
      </author>
      <author>
        <name>Chornock, R</name>
      </author>
      <author>
        <name>Chomiuk, L</name>
      </author>
      <author>
        <name>Copperwheat, CM</name>
      </author>
      <author>
        <name>Coughlin, MW</name>
      </author>
      <author>
        <name>Coppejans, DL</name>
      </author>
      <author>
        <name>Corsi, A</name>
      </author>
      <author>
        <name>D'Ammando, F</name>
      </author>
      <author>
        <name>Datrier, L</name>
      </author>
      <author>
        <name>D'Avanzo, P</name>
      </author>
      <author>
        <name>Dimitriadis, G</name>
      </author>
      <author>
        <name>Drout, MR</name>
      </author>
      <author>
        <name>Foley, RJ</name>
        <uri>https://orcid.org/0000-0002-2445-5275</uri>
      </author>
      <author>
        <name>Fong, W</name>
      </author>
      <author>
        <name>Fox, O</name>
      </author>
      <author>
        <name>Ghirlanda, G</name>
      </author>
      <author>
        <name>Goldstein, D</name>
      </author>
      <author>
        <name>Grindlay, J</name>
      </author>
      <author>
        <name>Guidorzi, C</name>
      </author>
      <author>
        <name>Haiman, Z</name>
      </author>
      <author>
        <name>Hendry, M</name>
      </author>
      <author>
        <name>Holz, D</name>
      </author>
      <author>
        <name>Hung, T</name>
      </author>
      <author>
        <name>Inserra, C</name>
      </author>
      <author>
        <name>Jones, DO</name>
      </author>
      <author>
        <name>Kalogera, V</name>
      </author>
      <author>
        <name>Kilpatrick, CD</name>
      </author>
      <author>
        <name>Lamb, G</name>
      </author>
      <author>
        <name>Laskar, T</name>
      </author>
      <author>
        <name>Levan, A</name>
      </author>
      <author>
        <name>Mason, E</name>
      </author>
      <author>
        <name>Maguire, K</name>
      </author>
      <author>
        <name>Melandri, A</name>
      </author>
      <author>
        <name>Milisavljevic, D</name>
      </author>
      <author>
        <name>Miller, A</name>
      </author>
      <author>
        <name>Narayan, G</name>
      </author>
      <author>
        <name>Nielsen, E</name>
      </author>
      <author>
        <name>Nicholl, M</name>
      </author>
      <author>
        <name>Nissanke, S</name>
      </author>
      <author>
        <name>Nugent, P</name>
        <uri>https://orcid.org/0000-0002-3389-0586</uri>
      </author>
      <author>
        <name>Pan, Y-C</name>
      </author>
      <author>
        <name>Pasham, D</name>
      </author>
      <author>
        <name>Paterson, K</name>
      </author>
      <author>
        <name>Piranomonte, S</name>
      </author>
      <author>
        <name>Racusin, J</name>
      </author>
      <author>
        <name>Rest, A</name>
      </author>
      <author>
        <name>Righi, C</name>
      </author>
      <author>
        <name>Sand, D</name>
      </author>
      <author>
        <name>Seaman, R</name>
      </author>
      <author>
        <name>Scolnic, D</name>
      </author>
      <author>
        <name>Siellez, K</name>
      </author>
      <author>
        <name>Singer, L</name>
      </author>
      <author>
        <name>Szkody, P</name>
      </author>
      <author>
        <name>Smith, M</name>
      </author>
      <author>
        <name>Steeghs, D</name>
      </author>
      <author>
        <name>Sullivan, M</name>
      </author>
      <author>
        <name>Tanvir, N</name>
      </author>
      <author>
        <name>Terreran, G</name>
      </author>
      <author>
        <name>Trimble, V</name>
      </author>
      <author>
        <name>Valenti, S</name>
      </author>
      <author>
        <name>Transient, with the support of the LSST</name>
      </author>
      <author>
        <name>Collaboration, Variable Stars</name>
      </author>
    </item>
    <item>
      <title>Dark matter contribution to Galactic diffuse gamma ray emission</title>
      <link>https://escholarship.org/uc/item/0nv0t5jj</link>
      <description>Observations of diffuse Galactic gamma ray emission (DGE) by the Fermi Large Area Telescope (LAT) allow a detailed study of cosmic rays and the interstellar medium. However, diffuse emission models of the inner Galaxy underpredict the Fermi-LAT data at energies above a few GeV and hint at possible nonastrophysical sources including dark matter (DM) annihilations or decays. We present a study of the possible emission components from DM using the high-resolution Via Lactea II N-body simulation of a Milky Way—sized DM halo. We generate full-sky maps of DM annihilation and decay signals that include modeling of the adiabatic contraction of the host density profile, Sommerfeld-enhanced DM annihilations, p-wave annihilations, and decaying DM. We compare our results with the DGE models produced by the Fermi-LAT team over different sky regions, including the Galactic center, high Galactic latitudes, and the Galactic anticenter. This work provides possible smooth component templates of...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/0nv0t5jj</guid>
      <pubDate>Tue, 17 Sep 2019 00:00:00 +0000</pubDate>
      <author>
        <name>Yang, Lin F</name>
      </author>
      <author>
        <name>Silk, Joseph</name>
      </author>
      <author>
        <name>Szalay, Alexander S</name>
      </author>
      <author>
        <name>Wyse, Rosemary FG</name>
      </author>
      <author>
        <name>Bozek, Brandon</name>
      </author>
      <author>
        <name>Madau, Piero</name>
        <uri>https://orcid.org/0000-0002-6336-3293</uri>
      </author>
    </item>
    <item>
      <title>First cosmological results using Type Ia supernovae from the Dark Energy Survey: measurement of the Hubble constant</title>
      <link>https://escholarship.org/uc/item/3dm8b3vr</link>
      <description>ABSTRACT
                  We present an improved measurement of the Hubble constant (H0) using the ‘inverse distance ladder’ method, which adds the information from 207 Type Ia supernovae (SNe Ia) from the Dark Energy Survey (DES) at redshift 0.018 &amp;lt; z &amp;lt; 0.85 to existing distance measurements of 122 low-redshift (z &amp;lt; 0.07) SNe Ia (Low-z) and measurements of Baryon Acoustic Oscillations (BAOs). Whereas traditional measurements of H0 with SNe Ia use a distance ladder of parallax and Cepheid variable stars, the inverse distance ladder relies on absolute distance measurements from the BAOs to calibrate the intrinsic magnitude of the SNe Ia. We find H0&amp;nbsp;= 67.8&amp;nbsp;±&amp;nbsp;1.3&amp;nbsp;km s−1 Mpc−1 (statistical and systematic uncertainties, 68&amp;nbsp;per cent confidence). Our measurement makes minimal assumptions about the underlying cosmological model, and our analysis was blinded to reduce confirmation bias. We examine possible systematic uncertainties and all are below the...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/3dm8b3vr</guid>
      <pubDate>Thu, 12 Sep 2019 00:00:00 +0000</pubDate>
      <author>
        <name>Macaulay, E</name>
      </author>
      <author>
        <name>Nichol, RC</name>
      </author>
      <author>
        <name>Bacon, D</name>
      </author>
      <author>
        <name>Brout, D</name>
      </author>
      <author>
        <name>Davis, TM</name>
      </author>
      <author>
        <name>Zhang, B</name>
      </author>
      <author>
        <name>Bassett, BA</name>
      </author>
      <author>
        <name>Scolnic, D</name>
      </author>
      <author>
        <name>Möller, A</name>
      </author>
      <author>
        <name>D’Andrea, CB</name>
      </author>
      <author>
        <name>Hinton, SR</name>
      </author>
      <author>
        <name>Kessler, R</name>
      </author>
      <author>
        <name>Kim, AG</name>
        <uri>https://orcid.org/0000-0001-6315-8743</uri>
      </author>
      <author>
        <name>Lasker, J</name>
      </author>
      <author>
        <name>Lidman, C</name>
      </author>
      <author>
        <name>Sako, M</name>
      </author>
      <author>
        <name>Smith, M</name>
      </author>
      <author>
        <name>Sullivan, M</name>
      </author>
      <author>
        <name>Abbott, TMC</name>
      </author>
      <author>
        <name>Allam, S</name>
      </author>
      <author>
        <name>Annis, J</name>
      </author>
      <author>
        <name>Asorey, J</name>
      </author>
      <author>
        <name>Avila, S</name>
      </author>
      <author>
        <name>Bechtol, K</name>
      </author>
      <author>
        <name>Brooks, D</name>
      </author>
      <author>
        <name>Brown, P</name>
      </author>
      <author>
        <name>Burke, DL</name>
      </author>
      <author>
        <name>Calcino, J</name>
      </author>
      <author>
        <name>Rosell, A Carnero</name>
      </author>
      <author>
        <name>Carollo, D</name>
      </author>
      <author>
        <name>Kind, M Carrasco</name>
      </author>
      <author>
        <name>Carretero, J</name>
      </author>
      <author>
        <name>Castander, FJ</name>
      </author>
      <author>
        <name>Collett, T</name>
      </author>
      <author>
        <name>Crocce, M</name>
      </author>
      <author>
        <name>Cunha, CE</name>
      </author>
      <author>
        <name>da Costa, LN</name>
      </author>
      <author>
        <name>Davis, C</name>
      </author>
      <author>
        <name>De Vicente, J</name>
      </author>
      <author>
        <name>Diehl, HT</name>
      </author>
      <author>
        <name>Doel, P</name>
      </author>
      <author>
        <name>Drlica-Wagner, A</name>
      </author>
      <author>
        <name>Eifler, TF</name>
      </author>
      <author>
        <name>Estrada, J</name>
      </author>
      <author>
        <name>Evrard, AE</name>
      </author>
      <author>
        <name>Filippenko, AV</name>
        <uri>https://orcid.org/0000-0003-3460-0103</uri>
      </author>
      <author>
        <name>Finley, DA</name>
      </author>
      <author>
        <name>Flaugher, B</name>
      </author>
      <author>
        <name>Foley, RJ</name>
        <uri>https://orcid.org/0000-0002-2445-5275</uri>
      </author>
      <author>
        <name>Fosalba, P</name>
      </author>
      <author>
        <name>Frieman, J</name>
      </author>
      <author>
        <name>Galbany, L</name>
      </author>
      <author>
        <name>García-Bellido, J</name>
      </author>
      <author>
        <name>Gaztanaga, E</name>
      </author>
      <author>
        <name>Glazebrook, K</name>
      </author>
      <author>
        <name>González-Gaitán, S</name>
      </author>
      <author>
        <name>Gruen, D</name>
      </author>
      <author>
        <name>Gruendl, RA</name>
      </author>
      <author>
        <name>Gschwend, J</name>
      </author>
      <author>
        <name>Gutierrez, G</name>
      </author>
      <author>
        <name>Hartley, WG</name>
      </author>
      <author>
        <name>Hollowood, DL</name>
      </author>
      <author>
        <name>Honscheid, K</name>
      </author>
      <author>
        <name>Hoormann, JK</name>
      </author>
      <author>
        <name>Hoyle, B</name>
      </author>
      <author>
        <name>Huterer, D</name>
      </author>
      <author>
        <name>Jain, B</name>
      </author>
      <author>
        <name>James, DJ</name>
      </author>
      <author>
        <name>Jeltema, T</name>
      </author>
      <author>
        <name>Kasai, E</name>
      </author>
      <author>
        <name>Krause, E</name>
      </author>
      <author>
        <name>Kuehn, K</name>
      </author>
      <author>
        <name>Kuropatkin, N</name>
      </author>
      <author>
        <name>Lahav, O</name>
      </author>
      <author>
        <name>Lewis, GF</name>
      </author>
      <author>
        <name>Li, TS</name>
      </author>
      <author>
        <name>Lima, M</name>
      </author>
      <author>
        <name>Lin, H</name>
      </author>
      <author>
        <name>Maia, MAG</name>
      </author>
      <author>
        <name>Marshall, JL</name>
      </author>
      <author>
        <name>Martini, P</name>
      </author>
      <author>
        <name>Miquel, R</name>
      </author>
      <author>
        <name>Nugent, P</name>
        <uri>https://orcid.org/0000-0002-3389-0586</uri>
      </author>
      <author>
        <name>Palmese, A</name>
      </author>
      <author>
        <name>Pan, Y-C</name>
      </author>
      <author>
        <name>Plazas, AA</name>
      </author>
      <author>
        <name>Romer, AK</name>
      </author>
      <author>
        <name>Roodman, A</name>
      </author>
      <author>
        <name>Sanchez, E</name>
      </author>
      <author>
        <name>Scarpine, V</name>
      </author>
      <author>
        <name>Schindler, R</name>
      </author>
      <author>
        <name>Schubnell, M</name>
      </author>
      <author>
        <name>Serrano, S</name>
      </author>
      <author>
        <name>Sevilla-Noarbe, I</name>
      </author>
      <author>
        <name>Sharp, R</name>
      </author>
      <author>
        <name>Soares-Santos, M</name>
      </author>
      <author>
        <name>Sobreira, F</name>
      </author>
      <author>
        <name>Sommer, NE</name>
      </author>
      <author>
        <name>Suchyta, E</name>
      </author>
      <author>
        <name>Swann, E</name>
      </author>
    </item>
    <item>
      <title>The Spectral Evolution of AT 2018dyb and the Presence of Metal Lines in Tidal Disruption Events</title>
      <link>https://escholarship.org/uc/item/1h8042d2</link>
      <description>We present light curves and spectra of the tidal disruption event (TDE) ASASSN-18pg/AT 2018dyb spanning a period of one year. The event shows a plethora of strong emission lines, including the Balmer series, He ii, He i, and metal lines of O iii λ3760 and N iii λλ4100, 4640 (blended with He ii). The latter lines are consistent with originating from the Bowen fluorescence mechanism. By analyzing literature spectra of past events, we conclude that these lines are common in TDEs. The spectral diversity of optical TDEs is thus larger than previously thought and includes N-rich events besides H- and He-rich events. We study how the spectral lines evolve with time, by means of their width, relative strength, and velocity offsets. The velocity width of the lines starts at ∼13,000 km s-1 and decreases with time. The ratio of He ii to N iii increases with time. The same is true for ASASSN-14li, which has a very similar spectrum to AT 2018dyb but its lines are narrower by a factor of &amp;gt;2....</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/1h8042d2</guid>
      <pubDate>Wed, 28 Aug 2019 00:00:00 +0000</pubDate>
      <author>
        <name>Leloudas, Giorgos</name>
      </author>
      <author>
        <name>Dai, Lixin</name>
      </author>
      <author>
        <name>Arcavi, Iair</name>
      </author>
      <author>
        <name>Vreeswijk, Paul M</name>
      </author>
      <author>
        <name>Mockler, Brenna</name>
      </author>
      <author>
        <name>Roy, Rupak</name>
      </author>
      <author>
        <name>Malesani, Daniele B</name>
      </author>
      <author>
        <name>Schulze, Steve</name>
      </author>
      <author>
        <name>Wevers, Thomas</name>
      </author>
      <author>
        <name>Fraser, Morgan</name>
      </author>
      <author>
        <name>Ramirez-Ruiz, Enrico</name>
      </author>
      <author>
        <name>Auchettl, Katie</name>
      </author>
      <author>
        <name>Burke, Jamison</name>
      </author>
      <author>
        <name>Cannizzaro, Giacomo</name>
      </author>
      <author>
        <name>Charalampopoulos, Panos</name>
      </author>
      <author>
        <name>Chen, Ting-Wan</name>
      </author>
      <author>
        <name>Cikota, Aleksandar</name>
      </author>
      <author>
        <name>Della Valle, Massimo</name>
      </author>
      <author>
        <name>Galbany, Lluis</name>
      </author>
      <author>
        <name>Gromadzki, Mariusz</name>
      </author>
      <author>
        <name>Heintz, Kasper E</name>
      </author>
      <author>
        <name>Hiramatsu, Daichi</name>
      </author>
      <author>
        <name>Jonker, Peter G</name>
      </author>
      <author>
        <name>Kostrzewa-Rutkowska, Zuzanna</name>
      </author>
      <author>
        <name>Maguire, Kate</name>
      </author>
      <author>
        <name>Mandel, Ilya</name>
      </author>
      <author>
        <name>Nicholl, Matt</name>
      </author>
      <author>
        <name>Onori, Francesca</name>
      </author>
      <author>
        <name>Roth, Nathaniel</name>
      </author>
      <author>
        <name>Smartt, Stephen J</name>
      </author>
      <author>
        <name>Wyrzykowski, Lukasz</name>
      </author>
      <author>
        <name>Young, Dave R</name>
      </author>
    </item>
    <item>
      <title>Less absorbed solar energy and more internal heat for Jupiter</title>
      <link>https://escholarship.org/uc/item/8p3609m8</link>
      <description>The radiant energy budget and internal heat are fundamental properties of giant planets, but precise determination of these properties remains a challenge. Here, we report measurements of Jupiter’s radiant energy budget and internal heat based on Cassini multi-instrument observations. Our findings reveal that Jupiter’s Bond albedo and internal heat, 0.503 ± 0.012 and 7.485 ± 0.160 W m−2 respectively, are significantly larger than 0.343 ± 0.032 and 5.444 ± 0.425 Wm−2, the previous best estimates. The new results help constrain and improve the current evolutionary theories and models for Jupiter. Furthermore, the significant wavelength dependency of Jupiter’s albedo implies that the radiant energy budgets and internal heat of the other giant planets in our solar system should be re-examined. Finally, the data sets of Jupiter’s characteristics of reflective solar spectral irradiance provide an observational basis for the models of giant exoplanets.</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/8p3609m8</guid>
      <pubDate>Mon, 26 Aug 2019 00:00:00 +0000</pubDate>
      <author>
        <name>Li, Liming</name>
      </author>
      <author>
        <name>Jiang, X</name>
      </author>
      <author>
        <name>West, RA</name>
      </author>
      <author>
        <name>Gierasch, PJ</name>
      </author>
      <author>
        <name>Perez-Hoyos, S</name>
      </author>
      <author>
        <name>Sanchez-Lavega, A</name>
      </author>
      <author>
        <name>Fletcher, LN</name>
      </author>
      <author>
        <name>Fortney, JJ</name>
        <uri>https://orcid.org/0000-0002-9843-4354</uri>
      </author>
      <author>
        <name>Knowles, B</name>
      </author>
      <author>
        <name>Porco, CC</name>
      </author>
      <author>
        <name>Baines, KH</name>
      </author>
      <author>
        <name>Fry, PM</name>
      </author>
      <author>
        <name>Mallama, A</name>
      </author>
      <author>
        <name>Achterberg, RK</name>
      </author>
      <author>
        <name>Simon, AA</name>
      </author>
      <author>
        <name>Nixon, CA</name>
      </author>
      <author>
        <name>Orton, GS</name>
      </author>
      <author>
        <name>Dyudina, UA</name>
      </author>
      <author>
        <name>Ewald, SP</name>
      </author>
      <author>
        <name>Schmude, RW</name>
      </author>
    </item>
    <item>
      <title>First cosmology results using Type Ia supernova from the Dark Energy Survey: simulations to correct supernova distance biases</title>
      <link>https://escholarship.org/uc/item/7838q8s3</link>
      <description>We describe catalogue-level simulations of Type Ia supernova (SN Ia) light curves in the Dark Energy Survey Supernova Program (DES-SN) and in low-redshift samples from the Center for Astrophysics (CfA) and the Carnegie Supernova Project (CSP). These simulations are used to model biases from selection effects and light-curve analysis and to determine bias corrections for SN Ia distance moduli that are used to measure cosmological parameters. To generate realistic light curves, the simulation uses a detailed SN Ia model, incorporates information from observations (point spread function, sky noise, zero-point), and uses summary information (e.g. detection efficiency versus signal-to-noise ratio) based on 10 000 fake SN light curves whose fluxes were overlaid on images and processed with our analysis pipelines. The quality of the simulation is illustrated by predicting distributions observed in the data. Averaging within redshift bins, we find distance modulus biases up to 0.05 mag...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/7838q8s3</guid>
      <pubDate>Tue, 6 Aug 2019 00:00:00 +0000</pubDate>
      <author>
        <name>Kessler, R</name>
      </author>
      <author>
        <name>Brout, D</name>
      </author>
      <author>
        <name>D’Andrea, CB</name>
      </author>
      <author>
        <name>Davis, TM</name>
      </author>
      <author>
        <name>Hinton, SR</name>
      </author>
      <author>
        <name>Kim, AG</name>
        <uri>https://orcid.org/0000-0001-6315-8743</uri>
      </author>
      <author>
        <name>Lasker, J</name>
      </author>
      <author>
        <name>Lidman, C</name>
      </author>
      <author>
        <name>Macaulay, E</name>
      </author>
      <author>
        <name>Möller, A</name>
      </author>
      <author>
        <name>Sako, M</name>
      </author>
      <author>
        <name>Scolnic, D</name>
      </author>
      <author>
        <name>Smith, M</name>
      </author>
      <author>
        <name>Sullivan, M</name>
      </author>
      <author>
        <name>Zhang, B</name>
      </author>
      <author>
        <name>Andersen, P</name>
      </author>
      <author>
        <name>Asorey, J</name>
      </author>
      <author>
        <name>Avelino, A</name>
      </author>
      <author>
        <name>Calcino, J</name>
      </author>
      <author>
        <name>Carollo, D</name>
      </author>
      <author>
        <name>Challis, P</name>
      </author>
      <author>
        <name>Childress, M</name>
      </author>
      <author>
        <name>Clocchiatti, A</name>
      </author>
      <author>
        <name>Crawford, S</name>
      </author>
      <author>
        <name>Filippenko, AV</name>
        <uri>https://orcid.org/0000-0003-3460-0103</uri>
      </author>
      <author>
        <name>Foley, RJ</name>
        <uri>https://orcid.org/0000-0002-2445-5275</uri>
      </author>
      <author>
        <name>Glazebrook, K</name>
      </author>
      <author>
        <name>Hoormann, JK</name>
      </author>
      <author>
        <name>Kasai, E</name>
      </author>
      <author>
        <name>Kirshner, RP</name>
      </author>
      <author>
        <name>Lewis, GF</name>
      </author>
      <author>
        <name>Mandel, KS</name>
      </author>
      <author>
        <name>March, M</name>
      </author>
      <author>
        <name>Morganson, E</name>
      </author>
      <author>
        <name>Muthukrishna, D</name>
      </author>
      <author>
        <name>Nugent, P</name>
        <uri>https://orcid.org/0000-0002-3389-0586</uri>
      </author>
      <author>
        <name>Pan, Y-C</name>
      </author>
      <author>
        <name>Sommer, NE</name>
      </author>
      <author>
        <name>Swann, E</name>
      </author>
      <author>
        <name>Thomas, RC</name>
      </author>
      <author>
        <name>Tucker, BE</name>
      </author>
      <author>
        <name>Uddin, SA</name>
      </author>
      <author>
        <name>Abbott, TMC</name>
      </author>
      <author>
        <name>Allam, S</name>
      </author>
      <author>
        <name>Annis, J</name>
      </author>
      <author>
        <name>Avila, S</name>
      </author>
      <author>
        <name>Banerji, M</name>
      </author>
      <author>
        <name>Bechtol, K</name>
      </author>
      <author>
        <name>Bertin, E</name>
      </author>
      <author>
        <name>Brooks, D</name>
      </author>
      <author>
        <name>Buckley-Geer, E</name>
      </author>
      <author>
        <name>Burke, DL</name>
      </author>
      <author>
        <name>Rosell, A Carnero</name>
      </author>
      <author>
        <name>Kind, M Carrasco</name>
      </author>
      <author>
        <name>Carretero, J</name>
      </author>
      <author>
        <name>Castander, FJ</name>
      </author>
      <author>
        <name>Crocce, M</name>
      </author>
      <author>
        <name>da Costa, LN</name>
      </author>
      <author>
        <name>Davis, C</name>
      </author>
      <author>
        <name>De Vicente, J</name>
      </author>
      <author>
        <name>Desai, S</name>
      </author>
      <author>
        <name>Diehl, HT</name>
      </author>
      <author>
        <name>Doel, P</name>
      </author>
      <author>
        <name>Eifler, TF</name>
      </author>
      <author>
        <name>Flaugher, B</name>
      </author>
      <author>
        <name>Fosalba, P</name>
      </author>
      <author>
        <name>Frieman, J</name>
      </author>
      <author>
        <name>García-Bellido, J</name>
      </author>
      <author>
        <name>Gaztanaga, E</name>
      </author>
      <author>
        <name>Gerdes, DW</name>
      </author>
      <author>
        <name>Gruen, D</name>
      </author>
      <author>
        <name>Gruendl, RA</name>
      </author>
      <author>
        <name>Gutierrez, G</name>
      </author>
      <author>
        <name>Hartley, WG</name>
      </author>
      <author>
        <name>Hollowood, DL</name>
      </author>
      <author>
        <name>Honscheid, K</name>
      </author>
      <author>
        <name>James, DJ</name>
      </author>
      <author>
        <name>Johnson, MWG</name>
      </author>
      <author>
        <name>Johnson, MD</name>
      </author>
      <author>
        <name>Krause, E</name>
      </author>
      <author>
        <name>Kuehn, K</name>
      </author>
      <author>
        <name>Kuropatkin, N</name>
      </author>
      <author>
        <name>Lahav, O</name>
      </author>
      <author>
        <name>Li, TS</name>
      </author>
      <author>
        <name>Lima, M</name>
      </author>
      <author>
        <name>Marshall, JL</name>
      </author>
      <author>
        <name>Martini, P</name>
      </author>
      <author>
        <name>Menanteau, F</name>
      </author>
      <author>
        <name>Miller, CJ</name>
      </author>
      <author>
        <name>Miquel, R</name>
      </author>
      <author>
        <name>Nord, B</name>
      </author>
      <author>
        <name>Plazas, AA</name>
      </author>
      <author>
        <name>Roodman, A</name>
      </author>
      <author>
        <name>Sanchez, E</name>
      </author>
      <author>
        <name>Scarpine, V</name>
      </author>
      <author>
        <name>Schindler, R</name>
      </author>
      <author>
        <name>Schubnell, M</name>
      </author>
      <author>
        <name>Serrano, S</name>
      </author>
      <author>
        <name>Sevilla-Noarbe, I</name>
      </author>
      <author>
        <name>Soares-Santos, M</name>
      </author>
    </item>
    <item>
      <title>Cosmological Constraints from Multiple Probes in the Dark Energy Survey</title>
      <link>https://escholarship.org/uc/item/63f2n75h</link>
      <description>The combination of multiple observational probes has long been advocated as a powerful technique to constrain cosmological parameters, in particular dark energy. The Dark Energy Survey has measured 207 spectroscopically confirmed type Ia supernova light curves, the baryon acoustic oscillation feature, weak gravitational lensing, and galaxy clustering. Here we present combined results from these probes, deriving constraints on the equation of state, w, of dark energy and its energy density in the Universe. Independently of other experiments, such as those that measure the cosmic microwave background, the probes from this single photometric survey rule out a Universe with no dark energy, finding w=-0.80_{-0.11}^{+0.09}. The geometry is shown to be consistent with a spatially flat Universe, and we obtain a constraint on the baryon density of Ω_{b}=0.069_{-0.012}^{+0.009} that is independent of early Universe measurements. These results demonstrate the potential power of large multiprobe...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/63f2n75h</guid>
      <pubDate>Tue, 6 Aug 2019 00:00:00 +0000</pubDate>
      <author>
        <name>Abbott, TMC</name>
      </author>
      <author>
        <name>Alarcon, A</name>
      </author>
      <author>
        <name>Allam, S</name>
      </author>
      <author>
        <name>Andersen, P</name>
      </author>
      <author>
        <name>Andrade-Oliveira, F</name>
      </author>
      <author>
        <name>Annis, J</name>
      </author>
      <author>
        <name>Asorey, J</name>
      </author>
      <author>
        <name>Avila, S</name>
      </author>
      <author>
        <name>Bacon, D</name>
      </author>
      <author>
        <name>Banik, N</name>
      </author>
      <author>
        <name>Bassett, BA</name>
      </author>
      <author>
        <name>Baxter, E</name>
      </author>
      <author>
        <name>Bechtol, K</name>
      </author>
      <author>
        <name>Becker, MR</name>
      </author>
      <author>
        <name>Bernstein, GM</name>
      </author>
      <author>
        <name>Bertin, E</name>
      </author>
      <author>
        <name>Blazek, J</name>
      </author>
      <author>
        <name>Bridle, SL</name>
      </author>
      <author>
        <name>Brooks, D</name>
      </author>
      <author>
        <name>Brout, D</name>
      </author>
      <author>
        <name>Burke, DL</name>
      </author>
      <author>
        <name>Calcino, J</name>
      </author>
      <author>
        <name>Camacho, H</name>
      </author>
      <author>
        <name>Campos, A</name>
      </author>
      <author>
        <name>Rosell, A Carnero</name>
      </author>
      <author>
        <name>Carollo, D</name>
      </author>
      <author>
        <name>Kind, M Carrasco</name>
      </author>
      <author>
        <name>Carretero, J</name>
      </author>
      <author>
        <name>Castander, FJ</name>
      </author>
      <author>
        <name>Cawthon, R</name>
      </author>
      <author>
        <name>Challis, P</name>
      </author>
      <author>
        <name>Chan, KC</name>
      </author>
      <author>
        <name>Chang, C</name>
      </author>
      <author>
        <name>Childress, M</name>
      </author>
      <author>
        <name>Crocce, M</name>
      </author>
      <author>
        <name>Cunha, CE</name>
      </author>
      <author>
        <name>D’Andrea, CB</name>
      </author>
      <author>
        <name>da Costa, LN</name>
      </author>
      <author>
        <name>Davis, C</name>
      </author>
      <author>
        <name>Davis, TM</name>
      </author>
      <author>
        <name>De Vicente, J</name>
      </author>
      <author>
        <name>DePoy, DL</name>
      </author>
      <author>
        <name>DeRose, J</name>
      </author>
      <author>
        <name>Desai, S</name>
      </author>
      <author>
        <name>Diehl, HT</name>
      </author>
      <author>
        <name>Dietrich, JP</name>
      </author>
      <author>
        <name>Dodelson, S</name>
      </author>
      <author>
        <name>Doel, P</name>
      </author>
      <author>
        <name>Drlica-Wagner, A</name>
      </author>
      <author>
        <name>Eifler, TF</name>
      </author>
      <author>
        <name>Elvin-Poole, J</name>
      </author>
      <author>
        <name>Estrada, J</name>
      </author>
      <author>
        <name>Evrard, AE</name>
      </author>
      <author>
        <name>Fernandez, E</name>
      </author>
      <author>
        <name>Flaugher, B</name>
      </author>
      <author>
        <name>Foley, RJ</name>
        <uri>https://orcid.org/0000-0002-2445-5275</uri>
      </author>
      <author>
        <name>Fosalba, P</name>
      </author>
      <author>
        <name>Frieman, J</name>
      </author>
      <author>
        <name>Galbany, L</name>
      </author>
      <author>
        <name>García-Bellido, J</name>
      </author>
      <author>
        <name>Gatti, M</name>
      </author>
      <author>
        <name>Gaztanaga, E</name>
      </author>
      <author>
        <name>Gerdes, DW</name>
      </author>
      <author>
        <name>Giannantonio, T</name>
      </author>
      <author>
        <name>Glazebrook, K</name>
      </author>
      <author>
        <name>Goldstein, DA</name>
      </author>
      <author>
        <name>Gruen, D</name>
      </author>
      <author>
        <name>Gruendl, RA</name>
      </author>
      <author>
        <name>Gschwend, J</name>
      </author>
      <author>
        <name>Gutierrez, G</name>
      </author>
      <author>
        <name>Hartley, WG</name>
      </author>
      <author>
        <name>Hinton, SR</name>
      </author>
      <author>
        <name>Hollowood, DL</name>
      </author>
      <author>
        <name>Honscheid, K</name>
      </author>
      <author>
        <name>Hoormann, JK</name>
      </author>
      <author>
        <name>Hoyle, B</name>
      </author>
      <author>
        <name>Huterer, D</name>
      </author>
      <author>
        <name>Jain, B</name>
      </author>
      <author>
        <name>James, DJ</name>
      </author>
      <author>
        <name>Jarvis, M</name>
      </author>
      <author>
        <name>Jeltema, T</name>
      </author>
      <author>
        <name>Kasai, E</name>
      </author>
      <author>
        <name>Kent, S</name>
      </author>
      <author>
        <name>Kessler, R</name>
      </author>
      <author>
        <name>Kim, AG</name>
        <uri>https://orcid.org/0000-0001-6315-8743</uri>
      </author>
      <author>
        <name>Kokron, N</name>
      </author>
      <author>
        <name>Krause, E</name>
      </author>
      <author>
        <name>Kron, R</name>
      </author>
      <author>
        <name>Kuehn, K</name>
      </author>
      <author>
        <name>Kuropatkin, N</name>
      </author>
      <author>
        <name>Lahav, O</name>
      </author>
      <author>
        <name>Lasker, J</name>
      </author>
      <author>
        <name>Lemos, P</name>
      </author>
      <author>
        <name>Lewis, GF</name>
      </author>
      <author>
        <name>Li, TS</name>
      </author>
      <author>
        <name>Lidman, C</name>
      </author>
      <author>
        <name>Lima, M</name>
      </author>
      <author>
        <name>Lin, H</name>
      </author>
      <author>
        <name>Macaulay, E</name>
      </author>
      <author>
        <name>MacCrann, N</name>
      </author>
    </item>
    <item>
      <title>Spatially Resolved Stellar Kinematics of the Ultra-diffuse Galaxy Dragonfly 44. II. Constraints on Fuzzy Dark Matter</title>
      <link>https://escholarship.org/uc/item/5982p41g</link>
      <description>Given the absence of directly detected dark matter (DM) as weakly interacting massive particles, there is strong interest in the possibility that DM is an ultralight scalar field, here denoted as "fuzzy" DM. Ultra-diffuse galaxies, with the sizes of giant galaxies and the luminosities of dwarf galaxies, have a wide range of DM halo masses, thus providing new opportunities for exploring the connections between galaxies and their DM halos. Following up on new integral field unit spectroscopic observations and dynamics modeling of the DM-dominated ultra-diffuse galaxy Dragonfly 44 in the outskirts of the Coma Cluster, we present models of fuzzy DM constrained by the stellar dynamics of this galaxy. We infer a scalar field mass of ∼ 3 × 10-22 eV, consistent with other constraints from galaxy dynamics but in tension with constraints from Lyα forest power spectrum modeling. While we are unable to statistically distinguish between fuzzy DM and "normal" cold DM models, we find that the...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/5982p41g</guid>
      <pubDate>Tue, 11 Jun 2019 00:00:00 +0000</pubDate>
      <author>
        <name>Wasserman, Asher</name>
      </author>
      <author>
        <name>van Dokkum, Pieter</name>
      </author>
      <author>
        <name>Romanowsky, Aaron J</name>
      </author>
      <author>
        <name>Brodie, Jean</name>
      </author>
      <author>
        <name>Danieli, Shany</name>
      </author>
      <author>
        <name>Forbes, Duncan A</name>
      </author>
      <author>
        <name>Abraham, Roberto</name>
      </author>
      <author>
        <name>Martin, Christopher</name>
      </author>
      <author>
        <name>Matuszewski, Matt</name>
      </author>
      <author>
        <name>Villaume, Alexa</name>
      </author>
      <author>
        <name>Tamanas, John</name>
      </author>
      <author>
        <name>Profumo, Stefano</name>
        <uri>https://orcid.org/0000-0002-9159-7556</uri>
      </author>
    </item>
    <item>
      <title>First Cosmology Results Using Type Ia Supernovae from the Dark Energy Survey: Photometric Pipeline and Light-curve Data Release</title>
      <link>https://escholarship.org/uc/item/5hs3g6st</link>
      <description>We present griz light curves of 251 SNe Ia from the first 3 years of the Dark Energy Survey Supernova Program’s (DES-SN) spectroscopically classified sample. The photometric pipeline described in this paper produces the calibrated fluxes and associated uncertainties used in the cosmological parameter analysis by employing a scene modeling approach that simultaneously models a variable transient flux and temporally constant host galaxy. We inject artificial point sources onto DECam images to test the accuracy of our photometric method. Upon comparison of input and measured artificial supernova fluxes, we find that flux biases peak at 3 mmag. We require corrections to our photometric uncertainties as a function of host galaxy surface brightness at the transient location, similar to that seen by the DES Difference Imaging Pipeline used to discover transients. The public release of the light curves can be found at https://des.ncsa.illinois.edu/releases/sn.</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/5hs3g6st</guid>
      <pubDate>Tue, 21 May 2019 00:00:00 +0000</pubDate>
      <author>
        <name>Brout, D</name>
      </author>
      <author>
        <name>Sako, M</name>
      </author>
      <author>
        <name>Scolnic, D</name>
      </author>
      <author>
        <name>Kessler, R</name>
      </author>
      <author>
        <name>D’Andrea, CB</name>
      </author>
      <author>
        <name>Davis, TM</name>
      </author>
      <author>
        <name>Hinton, SR</name>
      </author>
      <author>
        <name>Kim, AG</name>
        <uri>https://orcid.org/0000-0001-6315-8743</uri>
      </author>
      <author>
        <name>Lasker, J</name>
      </author>
      <author>
        <name>Macaulay, E</name>
      </author>
      <author>
        <name>Möller, A</name>
      </author>
      <author>
        <name>Nichol, RC</name>
      </author>
      <author>
        <name>Smith, M</name>
      </author>
      <author>
        <name>Sullivan, M</name>
      </author>
      <author>
        <name>Wolf, RC</name>
      </author>
      <author>
        <name>Allam, S</name>
      </author>
      <author>
        <name>Bassett, BA</name>
      </author>
      <author>
        <name>Brown, P</name>
      </author>
      <author>
        <name>Castander, FJ</name>
      </author>
      <author>
        <name>Childress, M</name>
      </author>
      <author>
        <name>Foley, RJ</name>
        <uri>https://orcid.org/0000-0002-2445-5275</uri>
      </author>
      <author>
        <name>Galbany, L</name>
      </author>
      <author>
        <name>Herner, K</name>
      </author>
      <author>
        <name>Kasai, E</name>
      </author>
      <author>
        <name>March, M</name>
      </author>
      <author>
        <name>Morganson, E</name>
      </author>
      <author>
        <name>Nugent, P</name>
        <uri>https://orcid.org/0000-0002-3389-0586</uri>
      </author>
      <author>
        <name>Pan, Y-C</name>
      </author>
      <author>
        <name>Thomas, RC</name>
      </author>
      <author>
        <name>Tucker, BE</name>
      </author>
      <author>
        <name>Wester, W</name>
      </author>
      <author>
        <name>Abbott, TMC</name>
      </author>
      <author>
        <name>Annis, J</name>
      </author>
      <author>
        <name>Avila, S</name>
      </author>
      <author>
        <name>Bertin, E</name>
      </author>
      <author>
        <name>Brooks, D</name>
      </author>
      <author>
        <name>Burke, DL</name>
      </author>
      <author>
        <name>Rosell, A Carnero</name>
      </author>
      <author>
        <name>Kind, M Carrasco</name>
      </author>
      <author>
        <name>Carretero, J</name>
      </author>
      <author>
        <name>Crocce, M</name>
      </author>
      <author>
        <name>Cunha, CE</name>
      </author>
      <author>
        <name>da Costa, LN</name>
      </author>
      <author>
        <name>Davis, C</name>
      </author>
      <author>
        <name>De Vicente, J</name>
      </author>
      <author>
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