Physical Sciences
Parent: Physical Sciences
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% |
| 867528n7 | DESI 2024: reconstructing dark energy using crossing statistics with DESI DR1 BAO data | 497 | 77 | 420 | 15.5% |
| 1946q35d | DESI 2024: Constraints on physics-focused aspects of dark energy using DESI DR1 BAO data | 491 | 312 | 179 | 63.5% |
| 2dt5w83t | DESI 2024 VI: cosmological constraints from the measurements of baryon acoustic oscillations | 487 | 88 | 399 | 18.1% |
| 28z4k02h | Constraints on neutrino physics from DESI DR2 BAO and DR1 full shape | 462 | 94 | 368 | 20.3% |
| 8xn4v0s5 | Dynamical dark energy in light of the DESI DR2 baryonic acoustic oscillations measurements | 449 | 220 | 229 | 49.0% |
| 6p44s2tv | Adiabatic matching of particle bunches in a plasma-based accelerator in the presence of ion motion | 421 | 355 | 66 | 84.3% |
| 10j633zs | A White Paper on keV sterile neutrino Dark Matter | 377 | 199 | 178 | 52.8% |
| 6dn8z4sg | Cosmological constraints from the cross-correlation of DESI Luminous Red Galaxies with CMB lensing from Planck PR4 and ACT DR6 | 366 | 275 | 91 | 75.1% |
| 2km4m4pj | The Robotic Multi-Object Focal Plane System of the Dark Energy Spectroscopic Instrument (DESI) | 355 | 221 | 134 | 62.3% |
| 1kp7z8tr | Laser-heated capillary discharge plasma waveguides for electron acceleration to 8 GeV | 346 | 234 | 112 | 67.6% |
| 55v7f7m0 | Plasma Guiding and Wakefield Generation for Second Generation Experiments | 340 | 302 | 38 | 88.8% |
| 2px009hq | Achievement of Target Gain Larger than Unity in an Inertial Fusion Experiment | 339 | 150 | 189 | 44.2% |
| 67q6j3gf | Cosmological implications of DESI DR2 BAO measurements in light of the latest ACT DR6 CMB data | 334 | 48 | 286 | 14.4% |
| 5mm917mq | Spontaneous fission of the odd-Z isotope Db255 | 318 | 185 | 133 | 58.2% |
| 3813v2ts | Stabilization and control of persistent current magnets using variable inductance | 314 | 150 | 164 | 47.8% |
| 8gg3z5b3 | DESI 2024 V: Full-Shape galaxy clustering from galaxies and quasars | 312 | 161 | 151 | 51.6% |
| 9zb2d29s | Mitigation of DESI fiber assignment incompleteness effect on two-point clustering with small angular scale truncated estimators | 296 | 229 | 67 | 77.4% |
| 6fc35504 | ELG spectroscopic systematics analysis of the DESI Data Release 1 | 295 | 218 | 77 | 73.9% |
| 0tc9r96f | Enhanced Isomer Population via Direct Irradiation of Solid-Density Targets Using a Compact Laser-Plasma Accelerator | 285 | 210 | 75 | 73.7% |
| 0fv331g6 | DESI DR2 results. II. Measurements of baryon acoustic oscillations and cosmological constraints | 283 | 0 | 283 | 0.0% |
| 0p92q5md | Toward the Discovery of New Elements: Production of Livermorium (Z=116) with Ti50 | 277 | 95 | 182 | 34.3% |
| 0rw8w2xf | Strong-field QED experiments using the BELLA PW laser dual beamlines | 277 | 131 | 146 | 47.3% |
| 3fx8c3xs | Multistage coupling of independent laser-plasma accelerators | 270 | 143 | 127 | 53.0% |
| 77n23236 | An accurate and efficient laser-envelope solver for the modeling of laser-plasma accelerators | 268 | 93 | 175 | 34.7% |
| 2ph3v80c | Plasma density gradient injection of low absolute momentum spread electron bunches | 263 | 36 | 227 | 13.7% |
| 538805vh | Diagnostics, Control and Performance Parameters for the BELLA High Repetition Rate Petawatt Class Laser | 263 | 215 | 48 | 81.7% |
| 79p4v28z | GeV electron beams from a cm-scale accelerator | 263 | 45 | 218 | 17.1% |
| 70w6x41n | The BABAR detector | 261 | 186 | 75 | 71.3% |
| 5502f0rk | A comparison between ShapeFit compression and Full-Modelling method with PyBird for DESI 2024 and beyond | 260 | 155 | 105 | 59.6% |
| 9x16p56f | Enhancing DESI DR1 full-shape analyses using HOD-informed priors | 260 | 207 | 53 | 79.6% |
| 6zh078qk | The DESI Early Data Release white dwarf catalogue | 254 | 172 | 82 | 67.7% |
| 8t474214 | Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Cosmological implications from two decades of spectroscopic surveys at the Apache Point Observatory | 253 | 168 | 85 | 66.4% |
| 07h356gd | Planning the Future of U.S. Particle Physics (Snowmass 2013): Chapter 8: Instrumentation Frontier | 251 | 154 | 97 | 61.4% |
| 28h344th | Mu2e Conceptual Design Report | 251 | 162 | 89 | 64.5% |
| 5217c2bm | Laser-heated capillary discharge waveguides as tunable structures for laser-plasma acceleration | 251 | 132 | 119 | 52.6% |
| 7nv6c95n | Constraining primordial non-Gaussianity with DESI 2024 LRG and QSO samples | 247 | 175 | 72 | 70.9% |
| 13045467 | Validating the galaxy and quasar catalog-level blinding scheme for the DESI 2024 analysis | 242 | 141 | 101 | 58.3% |
| 7wb5k8h5 | Characterization of a gamma-ray tracking array: A comparison of GRETINA and Gammasphere using a 60Co source | 239 | 144 | 95 | 60.3% |
| 46b0d4cc | Validation of the DESI DR2 measurements of baryon acoustic oscillations from galaxies and quasars | 238 | 0 | 238 | 0.0% |
| 85z0s9gh | New limits from microlensing on Galactic black holes in the mass range 10 M⊙ < M < 1000 M⊙ | 236 | 144 | 92 | 61.0% |
| 0z89g4qv | Fiducial-cosmology-dependent systematics for the DESI 2024 BAO analysis | 233 | 60 | 173 | 25.8% |
| 4338r7m1 | DESI Emission-line Galaxies: Clustering Dependence on Stellar Mass and [O II] Luminosity | 233 | 174 | 59 | 74.7% |
| 89c1q3cb | Multiple colliding laser pulses as a basis for studying high-field high-energy physics | 230 | 122 | 108 | 53.0% |
| 0778b8vd | Target Selection and Validation of DESI Quasars | 226 | 177 | 49 | 78.3% |
| 5681774p | A New Measurement of the Partial 0+->0+ Half Life of 10C with GAMMASPHERE | 225 | 47 | 178 | 20.9% |
| 1hz6q3jx | Comparative study of active plasma lenses in high-quality electron accelerator transport lines | 223 | 151 | 72 | 67.7% |
| 57v741p8 | The Simons Observatory: A fully remote controlled calibration system with a sparse wire grid for cosmic microwave background telescopes | 222 | 167 | 55 | 75.2% |
| 3jd3278g | Target Selection and Validation of DESI Emission Line Galaxies | 216 | 136 | 80 | 63.0% |
| 91g0w6f1 | The 13th Data Release of the Sloan Digital Sky Survey: First Spectroscopic Data from the SDSS-IV Survey Mapping Nearby Galaxies at Apache Point Observatory | 215 | 80 | 135 | 37.2% |
Note: Due to the evolving nature of web traffic, the data presented here should be considered approximate and subject to revision. Learn more.