Open Access Policy Deposits
Parent: Department of Astronomy and Astrophysics
eScholarship stats: Breakdown by Item for March through June, 2026
| Item | Title | Total requests | Download | View-only | %Dnld |
|---|---|---|---|---|---|
| 9j80t4m1 | The 16th Data Release of the Sloan Digital Sky Surveys: First Release from the APOGEE-2 Southern Survey and Full Release of eBOSS Spectra | 928 | 0 | 928 | 0.0% |
| 2zz1p7sc | SUPPLEMENT: “LOCALIZATION AND BROADBAND FOLLOW-UP OF THE GRAVITATIONAL-WAVE TRANSIENT GW150914” (2016, ApJL, 826, L13) | 880 | 706 | 174 | 80.2% |
| 82f057jt | Climate Action in Higher Education: Roadmap | 608 | 332 | 276 | 54.6% |
| 5v24p8hv | Multiwavelength constraints on the origin of a nearby repeating fast radio burst source in a globular cluster | 402 | 268 | 134 | 66.7% |
| 2qw2m22g | The Seventeenth Data Release of the Sloan Digital Sky Surveys: Complete Release of MaNGA, MaStar, and APOGEE-2 Data | 382 | 243 | 139 | 63.6% |
| 98c8s865 | The Palomar Transient Factory Core-collapse Supernova Host-galaxy Sample. I. Host-galaxy Distribution Functions and Environment Dependence of Core-collapse Supernovae | 333 | 253 | 80 | 76.0% |
| 4058w3z1 | Final Targeting Strategy for the Sloan Digital Sky Survey IV Apache Point Observatory Galactic Evolution Experiment 2 North Survey | 311 | 221 | 90 | 71.1% |
| 4059s5xd | A gravitational-wave standard siren measurement of the Hubble constant | 293 | 50 | 243 | 17.1% |
| 7fc5q0p2 | Search for Ultraheavy Dark Matter from Observations of Dwarf Spheroidal Galaxies with VERITAS | 291 | 154 | 137 | 52.9% |
| 11n957n7 | The TESS-Keck Survey. XVI. Mass Measurements for 12 Planets in Eight Systems | 290 | 197 | 93 | 67.9% |
| 11f44236 | THE DEEP2 GALAXY REDSHIFT SURVEY: DESIGN, OBSERVATIONS, DATA REDUCTION, AND REDSHIFTS**Based on observations taken at the W. M. Keck Observatory, which is operated jointly by the University of California and the California Institute of Technology, and on observations made with the NASA/ESO Hubble Space Telescope, obtained from the data archives at the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS5-26555, and from the Canadian Astronomy Data Centre. | 284 | 179 | 105 | 63.0% |
| 2tb3p8mk | LSST: From Science Drivers to Reference Design and Anticipated Data Products | 281 | 113 | 168 | 40.2% |
| 3h76z2tp | A tidal disruption event coincident with a high-energy neutrino | 270 | 168 | 102 | 62.2% |
| 0m5734s7 | Resolved imaging confirms a radiation belt around an ultracool dwarf | 269 | 77 | 192 | 28.6% |
| 50r7r20d | Multi-messenger Observations of a Binary Neutron Star Merger* * Any correspondence should be addressed to lvc.publications@ligo.org. | 264 | 69 | 195 | 26.1% |
| 4d77d3hk | The HETDEX Instrumentation: Hobby–Eberly Telescope Wide-field Upgrade and VIRUS | 263 | 147 | 116 | 55.9% |
| 6f8365cc | Saturn’s Probable Interior: An Exploration of Saturn’s Potential Interior Density Structures | 261 | 173 | 88 | 66.3% |
| 22f589zr | GRB 180620A: Evidence for Late-time Energy Injection | 255 | 156 | 99 | 61.2% |
| 84d0q763 | The Complete Light-curve Sample of Spectroscopically Confirmed SNe Ia from Pan-STARRS1 and Cosmological Constraints from the Combined Pantheon Sample | 253 | 121 | 132 | 47.8% |
| 77f6c5hq | SDSS-IV MaNGA: How the Stellar Populations of Passive Central Galaxies Depend on Stellar and Halo Mass | 251 | 153 | 98 | 61.0% |
| 0wc6v6pt | The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/Virgo GW170817. II. UV, Optical, and Near-infrared Light Curves and Comparison to Kilonova Models | 247 | 66 | 181 | 26.7% |
| 33q2b7z3 | Reimagining leadership through the everyday resistance of faculty of color. | 243 | 55 | 188 | 22.6% |
| 0vn7g57f | Saturn’s Probable Interior: An Exploration of Saturn’s Potential Interior Density Structures | 235 | 160 | 75 | 68.1% |
| 6nv5f7t1 | A trail of dark-matter-free galaxies from a bullet-dwarf collision | 235 | 60 | 175 | 25.5% |
| 9tc8q9vs | K2 Observations of SN 2018oh Reveal a Two-component Rising Light Curve for a Type Ia Supernova | 235 | 138 | 97 | 58.7% |
| 0f29389p | First Cosmology Results Using SNe Ia from the Dark Energy Survey: Analysis, Systematic Uncertainties, and Validation | 232 | 123 | 109 | 53.0% |
| 25h1s5ms | Identification of carbon dioxide in an exoplanet atmosphere | 231 | 94 | 137 | 40.7% |
| 7m06d2jp | GTC Follow-up Observations of Very Metal-poor Star Candidates from DESI | 226 | 104 | 122 | 46.0% |
| 8t30k6h1 | Multiwavelength follow-up of a rare IceCube neutrino multiplet | 221 | 120 | 101 | 54.3% |
| 6mh6q5hg | Giant Outer Transiting Exoplanet Mass (GOT ‘EM) Survey. V. Two Giant Planets in Kepler-511 but Only One Ran Away | 220 | 76 | 144 | 34.5% |
| 5m23m7m3 | ERRATUM: “AUTOMATED TRANSIENT IDENTIFICATION IN THE DARK ENERGY SURVEY” (2015, AJ, 150, 82) | 212 | 106 | 106 | 50.0% |
| 5616n854 | The Draco Dwarf Spheroidal Galaxy in the First Year of Dark Energy Spectroscopic Instrument Data | 211 | 68 | 143 | 32.2% |
| 8qb15891 | Optical and ultraviolet spectroscopic analysis of SN 2011fe at late times | 210 | 122 | 88 | 58.1% |
| 8xr2s1dv | Giant Outer Transiting Exoplanet Mass (GOT ‘EM) Survey. IV. Long-term Doppler Spectroscopy for 11 Stars Thought to Host Cool Giant Exoplanets | 207 | 129 | 78 | 62.3% |
| 38s3v07s | 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. | 205 | 120 | 85 | 58.5% |
| 05b81661 | Astrophysics. Multiple images of a highly magnified supernova formed by an early-type cluster galaxy lens. | 204 | 109 | 95 | 53.4% |
| 79d3m4h0 | The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/Virgo GW170817. IV. Detection of Near-infrared Signatures of r-process Nucleosynthesis with Gemini-South | 200 | 84 | 116 | 42.0% |
| 5hj1h0bf | The TESS-Keck Survey. II. An Ultra-short-period Rocky Planet and Its Siblings Transiting the Galactic Thick-disk Star TOI-561 | 199 | 80 | 119 | 40.2% |
| 7281k86f | The Magnificent Five Images of Supernova Refsdal: Time Delay and Magnification Measurements | 199 | 78 | 121 | 39.2% |
| 0v44n629 | Sloan Digital Sky Survey IV: Mapping the Milky Way, Nearby Galaxies, and the Distant Universe | 198 | 109 | 89 | 55.1% |
| 498713kh | The Dark Energy Survey: Cosmology Results with ∼1500 New High-redshift Type Ia Supernovae Using the Full 5 yr Data Set | 192 | 85 | 107 | 44.3% |
| 7gh663p7 | The Old Host-galaxy Environment of SSS17a, the First Electromagnetic Counterpart to a Gravitational-wave Source* * This paper includes data gathered with the 6.5 meter Magellan Telescopes located at Las Campanas Observatory, Chile. | 191 | 114 | 77 | 59.7% |
| 95s4v1hf | Discovery and Follow-up Observations of the Young Type Ia Supernova 2016coj | 190 | 136 | 54 | 71.6% |
| 3447b7h1 | TYPE Ia SUPERNOVA RATE MEASUREMENTS TO REDSHIFT 2.5 FROM CANDELS: SEARCHING FOR PROMPT EXPLOSIONS IN THE EARLY UNIVERSE | 189 | 86 | 103 | 45.5% |
| 8k19n0p9 | The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/Virgo GW170817. I. Discovery of the Optical Counterpart Using the Dark Energy Camera | 189 | 71 | 118 | 37.6% |
| 2xh2k163 | THE AGORA HIGH-RESOLUTION GALAXY SIMULATIONS COMPARISON PROJECT. II. ISOLATED DISK TEST | 187 | 92 | 95 | 49.2% |
| 90d3n6hc | Structural and Star-forming Relations since z similar to 3: Connecting Compact Star-forming and Quiescent Galaxies | 185 | 56 | 129 | 30.3% |
| 9ph804bp | A PANCHROMATIC VIEW OF THE RESTLESS SN 2009ip REVEALS THE EXPLOSIVE EJECTION OF A MASSIVE STAR ENVELOPE | 185 | 102 | 83 | 55.1% |
| 2f18c097 | Target of Opportunity Observations of Gravitational Wave Events with LSST | 183 | 85 | 98 | 46.4% |
| 3d5712fq | Multiple images of a highly magnified supernova formed by an early-type cluster galaxy lens | 183 | 110 | 73 | 60.1% |
Note: Due to the evolving nature of web traffic, the data presented here should be considered approximate and subject to revision. Learn more.