Open Access Policy Deposits
Parent: Department of Astronomy and Astrophysics
eScholarship stats: Breakdown by Item for May through August, 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 | 906 | 0 | 906 | 0.0% |
| 2zz1p7sc | SUPPLEMENT: “LOCALIZATION AND BROADBAND FOLLOW-UP OF THE GRAVITATIONAL-WAVE TRANSIENT GW150914” (2016, ApJL, 826, L13) | 534 | 391 | 143 | 73.2% |
| 5v24p8hv | Multiwavelength constraints on the origin of a nearby repeating fast radio burst source in a globular cluster | 475 | 315 | 160 | 66.3% |
| 82f057jt | Climate Action in Higher Education: Roadmap | 468 | 321 | 147 | 68.6% |
| 2qw2m22g | The Seventeenth Data Release of the Sloan Digital Sky Surveys: Complete Release of MaNGA, MaStar, and APOGEE-2 Data | 408 | 321 | 87 | 78.7% |
| 4058w3z1 | Final Targeting Strategy for the Sloan Digital Sky Survey IV Apache Point Observatory Galactic Evolution Experiment 2 North Survey | 383 | 310 | 73 | 80.9% |
| 50r7r20d | Multi-messenger Observations of a Binary Neutron Star Merger* * Any correspondence should be addressed to lvc.publications@ligo.org. | 383 | 62 | 321 | 16.2% |
| 98c8s865 | The Palomar Transient Factory Core-collapse Supernova Host-galaxy Sample. I. Host-galaxy Distribution Functions and Environment Dependence of Core-collapse Supernovae | 352 | 304 | 48 | 86.4% |
| 2tb3p8mk | LSST: From Science Drivers to Reference Design and Anticipated Data Products | 308 | 100 | 208 | 32.5% |
| 498713kh | The Dark Energy Survey: Cosmology Results with ∼1500 New High-redshift Type Ia Supernovae Using the Full 5 yr Data Set | 278 | 122 | 156 | 43.9% |
| 22f589zr | GRB 180620A: Evidence for Late-time Energy Injection | 272 | 186 | 86 | 68.4% |
| 3h76z2tp | A tidal disruption event coincident with a high-energy neutrino | 269 | 182 | 87 | 67.7% |
| 77f6c5hq | SDSS-IV MaNGA: How the Stellar Populations of Passive Central Galaxies Depend on Stellar and Halo Mass | 261 | 160 | 101 | 61.3% |
| 11n957n7 | The TESS-Keck Survey. XVI. Mass Measurements for 12 Planets in Eight Systems | 259 | 192 | 67 | 74.1% |
| 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. | 255 | 160 | 95 | 62.7% |
| 6mh6q5hg | Giant Outer Transiting Exoplanet Mass (GOT ‘EM) Survey. V. Two Giant Planets in Kepler-511 but Only One Ran Away | 253 | 77 | 176 | 30.4% |
| 4d77d3hk | The HETDEX Instrumentation: Hobby–Eberly Telescope Wide-field Upgrade and VIRUS | 252 | 156 | 96 | 61.9% |
| 7fc5q0p2 | Search for Ultraheavy Dark Matter from Observations of Dwarf Spheroidal Galaxies with VERITAS | 241 | 156 | 85 | 64.7% |
| 8t30k6h1 | Multiwavelength follow-up of a rare IceCube neutrino multiplet | 236 | 155 | 81 | 65.7% |
| 9tc8q9vs | K2 Observations of SN 2018oh Reveal a Two-component Rising Light Curve for a Type Ia Supernova | 235 | 147 | 88 | 62.6% |
| 6nv5f7t1 | A trail of dark-matter-free galaxies from a bullet-dwarf collision | 234 | 89 | 145 | 38.0% |
| 84d0q763 | The Complete Light-curve Sample of Spectroscopically Confirmed SNe Ia from Pan-STARRS1 and Cosmological Constraints from the Combined Pantheon Sample | 227 | 143 | 84 | 63.0% |
| 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 | 219 | 44 | 175 | 20.1% |
| 7838q8s3 | First cosmology results using Type Ia supernova from the Dark Energy Survey: simulations to correct supernova distance biases | 217 | 32 | 185 | 14.7% |
| 5m23m7m3 | ERRATUM: “AUTOMATED TRANSIENT IDENTIFICATION IN THE DARK ENERGY SURVEY” (2015, AJ, 150, 82) | 216 | 129 | 87 | 59.7% |
| 0m5734s7 | Resolved imaging confirms a radiation belt around an ultracool dwarf | 204 | 57 | 147 | 27.9% |
| 95s4v1hf | Discovery and Follow-up Observations of the Young Type Ia Supernova 2016coj | 204 | 140 | 64 | 68.6% |
| 0v44n629 | Sloan Digital Sky Survey IV: Mapping the Milky Way, Nearby Galaxies, and the Distant Universe | 202 | 71 | 131 | 35.1% |
| 0vn7g57f | Saturn’s Probable Interior: An Exploration of Saturn’s Potential Interior Density Structures | 202 | 138 | 64 | 68.3% |
| 0f29389p | First Cosmology Results Using SNe Ia from the Dark Energy Survey: Analysis, Systematic Uncertainties, and Validation | 200 | 133 | 67 | 66.5% |
| 2p84t4bs | The Hourglass Simulation: A Catalog for the Roman High-latitude Time-domain Core Community Survey | 197 | 80 | 117 | 40.6% |
| 8k19n0p9 | The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/Virgo GW170817. I. Discovery of the Optical Counterpart Using the Dark Energy Camera | 194 | 105 | 89 | 54.1% |
| 25h1s5ms | Identification of carbon dioxide in an exoplanet atmosphere | 188 | 82 | 106 | 43.6% |
| 33q2b7z3 | Reimagining leadership through the everyday resistance of faculty of color. | 188 | 49 | 139 | 26.1% |
| 8qb15891 | Optical and ultraviolet spectroscopic analysis of SN 2011fe at late times | 186 | 128 | 58 | 68.8% |
| 2xh2k163 | THE AGORA HIGH-RESOLUTION GALAXY SIMULATIONS COMPARISON PROJECT. II. ISOLATED DISK TEST | 185 | 111 | 74 | 60.0% |
| 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. | 181 | 130 | 51 | 71.8% |
| 6f8365cc | Saturn’s Probable Interior: An Exploration of Saturn’s Potential Interior Density Structures | 181 | 131 | 50 | 72.4% |
| 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. | 179 | 126 | 53 | 70.4% |
| 05b81661 | Astrophysics. Multiple images of a highly magnified supernova formed by an early-type cluster galaxy lens. | 176 | 105 | 71 | 59.7% |
| 3d5712fq | Multiple images of a highly magnified supernova formed by an early-type cluster galaxy lens | 176 | 135 | 41 | 76.7% |
| 9ph804bp | A PANCHROMATIC VIEW OF THE RESTLESS SN 2009ip REVEALS THE EXPLOSIVE EJECTION OF A MASSIVE STAR ENVELOPE | 170 | 115 | 55 | 67.6% |
| 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 | 169 | 83 | 86 | 49.1% |
| 4059s5xd | A gravitational-wave standard siren measurement of the Hubble constant | 166 | 35 | 131 | 21.1% |
| 8xr2s1dv | Giant Outer Transiting Exoplanet Mass (GOT ‘EM) Survey. IV. Long-term Doppler Spectroscopy for 11 Stars Thought to Host Cool Giant Exoplanets | 165 | 109 | 56 | 66.1% |
| 90d3n6hc | Structural and Star-forming Relations since z similar to 3: Connecting Compact Star-forming and Quiescent Galaxies | 161 | 60 | 101 | 37.3% |
| 3db4r31q | The Need for Laboratory Measurements and Ab Initio Studies to Aid Understanding of Exoplanetary Atmospheres | 156 | 31 | 125 | 19.9% |
| 1g07f9c8 | Reverse Shock Emission Revealed in Early Photometry in the Candidate Short GRB 180418A | 154 | 96 | 58 | 62.3% |
| 41t078q9 | Studying the Ultraviolet Spectrum of the First Spectroscopically Confirmed Supernova at Redshift Two | 153 | 34 | 119 | 22.2% |
| 3447b7h1 | TYPE Ia SUPERNOVA RATE MEASUREMENTS TO REDSHIFT 2.5 FROM CANDELS: SEARCHING FOR PROMPT EXPLOSIONS IN THE EARLY UNIVERSE | 148 | 72 | 76 | 48.6% |
Note: Due to the evolving nature of web traffic, the data presented here should be considered approximate and subject to revision. Learn more.