Open Access Policy Deposits
Parent: Department of Astronomy and Astrophysics
eScholarship stats: Breakdown by Item for July through October, 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 | 610 | 0 | 610 | 0.0% |
| 2qw2m22g | The Seventeenth Data Release of the Sloan Digital Sky Surveys: Complete Release of MaNGA, MaStar, and APOGEE-2 Data | 563 | 504 | 59 | 89.5% |
| 50r7r20d | Multi-messenger Observations of a Binary Neutron Star Merger* * Any correspondence should be addressed to lvc.publications@ligo.org. | 452 | 95 | 357 | 21.0% |
| 5v24p8hv | Multiwavelength constraints on the origin of a nearby repeating fast radio burst source in a globular cluster | 446 | 318 | 128 | 71.3% |
| 4058w3z1 | Final Targeting Strategy for the Sloan Digital Sky Survey IV Apache Point Observatory Galactic Evolution Experiment 2 North Survey | 408 | 350 | 58 | 85.8% |
| 98c8s865 | The Palomar Transient Factory Core-collapse Supernova Host-galaxy Sample. I. Host-galaxy Distribution Functions and Environment Dependence of Core-collapse Supernovae | 408 | 344 | 64 | 84.3% |
| 82f057jt | Climate Action in Higher Education: Roadmap | 390 | 251 | 139 | 64.4% |
| 4d77d3hk | The HETDEX Instrumentation: Hobby–Eberly Telescope Wide-field Upgrade and VIRUS | 365 | 273 | 92 | 74.8% |
| 77f6c5hq | SDSS-IV MaNGA: How the Stellar Populations of Passive Central Galaxies Depend on Stellar and Halo Mass | 328 | 246 | 82 | 75.0% |
| 498713kh | The Dark Energy Survey: Cosmology Results with ∼1500 New High-redshift Type Ia Supernovae Using the Full 5 yr Data Set | 323 | 144 | 179 | 44.6% |
| 9tc8q9vs | K2 Observations of SN 2018oh Reveal a Two-component Rising Light Curve for a Type Ia Supernova | 319 | 241 | 78 | 75.5% |
| 3h76z2tp | A tidal disruption event coincident with a high-energy neutrino | 303 | 251 | 52 | 82.8% |
| 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. | 302 | 258 | 44 | 85.4% |
| 22f589zr | GRB 180620A: Evidence for Late-time Energy Injection | 296 | 230 | 66 | 77.7% |
| 7fc5q0p2 | Search for Ultraheavy Dark Matter from Observations of Dwarf Spheroidal Galaxies with VERITAS | 296 | 245 | 51 | 82.8% |
| 84d0q763 | The Complete Light-curve Sample of Spectroscopically Confirmed SNe Ia from Pan-STARRS1 and Cosmological Constraints from the Combined Pantheon Sample | 284 | 244 | 40 | 85.9% |
| 8t30k6h1 | Multiwavelength follow-up of a rare IceCube neutrino multiplet | 282 | 213 | 69 | 75.5% |
| 6mh6q5hg | Giant Outer Transiting Exoplanet Mass (GOT ‘EM) Survey. V. Two Giant Planets in Kepler-511 but Only One Ran Away | 259 | 94 | 165 | 36.3% |
| 1g07f9c8 | Reverse Shock Emission Revealed in Early Photometry in the Candidate Short GRB 180418A | 257 | 206 | 51 | 80.2% |
| 95s4v1hf | Discovery and Follow-up Observations of the Young Type Ia Supernova 2016coj | 229 | 183 | 46 | 79.9% |
| 2tb3p8mk | LSST: From Science Drivers to Reference Design and Anticipated Data Products | 222 | 76 | 146 | 34.2% |
| 2p84t4bs | The Hourglass Simulation: A Catalog for the Roman High-latitude Time-domain Core Community Survey | 216 | 58 | 158 | 26.9% |
| 7838q8s3 | First cosmology results using Type Ia supernova from the Dark Energy Survey: simulations to correct supernova distance biases | 216 | 22 | 194 | 10.2% |
| 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. | 214 | 99 | 115 | 46.3% |
| 8cx2g916 | Multidimensional Radiation Hydrodynamics Simulations of Pulsational Pair-instability Supernovae | 211 | 162 | 49 | 76.8% |
| 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. | 209 | 172 | 37 | 82.3% |
| 0v44n629 | Sloan Digital Sky Survey IV: Mapping the Milky Way, Nearby Galaxies, and the Distant Universe | 207 | 68 | 139 | 32.9% |
| 5m23m7m3 | ERRATUM: “AUTOMATED TRANSIENT IDENTIFICATION IN THE DARK ENERGY SURVEY” (2015, AJ, 150, 82) | 207 | 162 | 45 | 78.3% |
| 6nv5f7t1 | A trail of dark-matter-free galaxies from a bullet-dwarf collision | 195 | 89 | 106 | 45.6% |
| 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 | 177 | 27 | 150 | 15.3% |
| 2zz1p7sc | SUPPLEMENT: “LOCALIZATION AND BROADBAND FOLLOW-UP OF THE GRAVITATIONAL-WAVE TRANSIENT GW150914” (2016, ApJL, 826, L13) | 177 | 115 | 62 | 65.0% |
| 2f18c097 | Target of Opportunity Observations of Gravitational Wave Events with LSST | 176 | 139 | 37 | 79.0% |
| 8k19n0p9 | The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/Virgo GW170817. I. Discovery of the Optical Counterpart Using the Dark Energy Camera | 174 | 121 | 53 | 69.5% |
| 9ph804bp | A PANCHROMATIC VIEW OF THE RESTLESS SN 2009ip REVEALS THE EXPLOSIVE EJECTION OF A MASSIVE STAR ENVELOPE | 173 | 114 | 59 | 65.9% |
| 2xh2k163 | THE AGORA HIGH-RESOLUTION GALAXY SIMULATIONS COMPARISON PROJECT. II. ISOLATED DISK TEST | 165 | 88 | 77 | 53.3% |
| 8qb15891 | Optical and ultraviolet spectroscopic analysis of SN 2011fe at late times | 162 | 117 | 45 | 72.2% |
| 0f29389p | First Cosmology Results Using SNe Ia from the Dark Energy Survey: Analysis, Systematic Uncertainties, and Validation | 161 | 105 | 56 | 65.2% |
| 1rs528tc | LSST Observing Strategy White Paper: LSST Observations of WFIRST Deep Fields | 152 | 91 | 61 | 59.9% |
| 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 | 150 | 88 | 62 | 58.7% |
| 63f2n75h | Cosmological Constraints from Multiple Probes in the Dark Energy Survey | 149 | 53 | 96 | 35.6% |
| 11n957n7 | The TESS-Keck Survey. XVI. Mass Measurements for 12 Planets in Eight Systems | 147 | 90 | 57 | 61.2% |
| 1fx8c7sr | A DECAM SEARCH FOR AN OPTICAL COUNTERPART TO THE LIGO GRAVITATIONAL-WAVE EVENT GW151226 | 147 | 73 | 74 | 49.7% |
| 33q2b7z3 | Reimagining leadership through the everyday resistance of faculty of color. | 143 | 39 | 104 | 27.3% |
| 3d5712fq | Multiple images of a highly magnified supernova formed by an early-type cluster galaxy lens | 143 | 105 | 38 | 73.4% |
| 05b81661 | Astrophysics. Multiple images of a highly magnified supernova formed by an early-type cluster galaxy lens. | 142 | 90 | 52 | 63.4% |
| 6f8365cc | Saturn’s Probable Interior: An Exploration of Saturn’s Potential Interior Density Structures | 140 | 93 | 47 | 66.4% |
| 0vn7g57f | Saturn’s Probable Interior: An Exploration of Saturn’s Potential Interior Density Structures | 137 | 91 | 46 | 66.4% |
| 90d3n6hc | Structural and Star-forming Relations since z similar to 3: Connecting Compact Star-forming and Quiescent Galaxies | 137 | 60 | 77 | 43.8% |
| 0fq714g1 | Evidence That the Directly Imaged Planet HD 131399 Ab Is a Background Star | 135 | 62 | 73 | 45.9% |
| 8p3609m8 | Less absorbed solar energy and more internal heat for Jupiter | 133 | 60 | 73 | 45.1% |
Note: Due to the evolving nature of web traffic, the data presented here should be considered approximate and subject to revision. Learn more.