Physical Sciences
Parent: Physical Sciences
eScholarship stats: Breakdown by Item for June through September, 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 | 793 | 0 | 793 | 0.0% |
| 28z4k02h | Constraints on neutrino physics from DESI DR2 BAO and DR1 full shape | 503 | 89 | 414 | 17.7% |
| 2dt5w83t | DESI 2024 VI: cosmological constraints from the measurements of baryon acoustic oscillations | 456 | 56 | 400 | 12.3% |
| 867528n7 | DESI 2024: reconstructing dark energy using crossing statistics with DESI DR1 BAO data | 428 | 58 | 370 | 13.6% |
| 1946q35d | DESI 2024: Constraints on physics-focused aspects of dark energy using DESI DR1 BAO data | 418 | 249 | 169 | 59.6% |
| 8xn4v0s5 | Dynamical dark energy in light of the DESI DR2 baryonic acoustic oscillations measurements | 410 | 172 | 238 | 42.0% |
| 67q6j3gf | Cosmological implications of DESI DR2 BAO measurements in light of the latest ACT DR6 CMB data | 351 | 51 | 300 | 14.5% |
| 2px009hq | Achievement of Target Gain Larger than Unity in an Inertial Fusion Experiment | 348 | 161 | 187 | 46.3% |
| 6p44s2tv | Adiabatic matching of particle bunches in a plasma-based accelerator in the presence of ion motion | 340 | 269 | 71 | 79.1% |
| 55v7f7m0 | Plasma Guiding and Wakefield Generation for Second Generation Experiments | 336 | 306 | 30 | 91.1% |
| 8gg3z5b3 | DESI 2024 V: Full-Shape galaxy clustering from galaxies and quasars | 327 | 126 | 201 | 38.5% |
| 5mm917mq | Spontaneous fission of the odd-Z isotope Db255 | 316 | 180 | 136 | 57.0% |
| 10j633zs | A White Paper on keV sterile neutrino Dark Matter | 311 | 162 | 149 | 52.1% |
| 6dn8z4sg | Cosmological constraints from the cross-correlation of DESI Luminous Red Galaxies with CMB lensing from Planck PR4 and ACT DR6 | 309 | 211 | 98 | 68.3% |
| 0fv331g6 | DESI DR2 results. II. Measurements of baryon acoustic oscillations and cosmological constraints | 279 | 0 | 279 | 0.0% |
| 2km4m4pj | The Robotic Multi-Object Focal Plane System of the Dark Energy Spectroscopic Instrument (DESI) | 272 | 158 | 114 | 58.1% |
| 1kp7z8tr | Laser-heated capillary discharge plasma waveguides for electron acceleration to 8 GeV | 267 | 192 | 75 | 71.9% |
| 2ph3v80c | Plasma density gradient injection of low absolute momentum spread electron bunches | 258 | 32 | 226 | 12.4% |
| 20d8g0hb | Ion acceleration in laser generated megatesla magnetic vortex | 254 | 48 | 206 | 18.9% |
| 5217c2bm | Laser-heated capillary discharge waveguides as tunable structures for laser-plasma acceleration | 254 | 130 | 124 | 51.2% |
| 9zb2d29s | Mitigation of DESI fiber assignment incompleteness effect on two-point clustering with small angular scale truncated estimators | 251 | 196 | 55 | 78.1% |
| 46b0d4cc | Validation of the DESI DR2 measurements of baryon acoustic oscillations from galaxies and quasars | 248 | 0 | 248 | 0.0% |
| 538805vh | Diagnostics, Control and Performance Parameters for the BELLA High Repetition Rate Petawatt Class Laser | 248 | 192 | 56 | 77.4% |
| 6fc35504 | ELG spectroscopic systematics analysis of the DESI Data Release 1 | 247 | 194 | 53 | 78.5% |
| 0p92q5md | Toward the Discovery of New Elements: Production of Livermorium (Z=116) with Ti50 | 246 | 72 | 174 | 29.3% |
| 0tc9r96f | Enhanced Isomer Population via Direct Irradiation of Solid-Density Targets Using a Compact Laser-Plasma Accelerator | 242 | 177 | 65 | 73.1% |
| 3813v2ts | Stabilization and control of persistent current magnets using variable inductance | 237 | 118 | 119 | 49.8% |
| 79p4v28z | GeV electron beams from a cm-scale accelerator | 236 | 31 | 205 | 13.1% |
| 07h356gd | Planning the Future of U.S. Particle Physics (Snowmass 2013): Chapter 8: Instrumentation Frontier | 233 | 142 | 91 | 60.9% |
| 3fx8c3xs | Multistage coupling of independent laser-plasma accelerators | 231 | 136 | 95 | 58.9% |
| 70w6x41n | The BABAR detector | 225 | 144 | 81 | 64.0% |
| 77n23236 | An accurate and efficient laser-envelope solver for the modeling of laser-plasma accelerators | 225 | 59 | 166 | 26.2% |
| 7nv6c95n | Constraining primordial non-Gaussianity with DESI 2024 LRG and QSO samples | 222 | 139 | 83 | 62.6% |
| 7wd7c75m | Publisher’s Note: Decay and Fission Hindrance of Two- and Four-Quasiparticle K Isomers in Rf254 [Phys. Rev. Lett. 115, 132502 (2015)] | 221 | 109 | 112 | 49.3% |
| 28h344th | Mu2e Conceptual Design Report | 219 | 159 | 60 | 72.6% |
| 0z89g4qv | Fiducial-cosmology-dependent systematics for the DESI 2024 BAO analysis | 217 | 25 | 192 | 11.5% |
| 6zh078qk | The DESI Early Data Release white dwarf catalogue | 215 | 134 | 81 | 62.3% |
| 9x16p56f | Enhancing DESI DR1 full-shape analyses using HOD-informed priors | 215 | 173 | 42 | 80.5% |
| 8t474214 | Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Cosmological implications from two decades of spectroscopic surveys at the Apache Point Observatory | 213 | 147 | 66 | 69.0% |
| 5502f0rk | A comparison between ShapeFit compression and Full-Modelling method with PyBird for DESI 2024 and beyond | 212 | 136 | 76 | 64.2% |
| 1qx8n794 | Constraints on primordial non-Gaussianity from the cross-correlation of DESI luminous red galaxies and Planck CMB lensing | 211 | 45 | 166 | 21.3% |
| 89c1q3cb | Multiple colliding laser pulses as a basis for studying high-field high-energy physics | 211 | 105 | 106 | 49.8% |
| 7wb5k8h5 | Characterization of a gamma-ray tracking array: A comparison of GRETINA and Gammasphere using a 60Co source | 208 | 124 | 84 | 59.6% |
| 5681774p | A New Measurement of the Partial 0+->0+ Half Life of 10C with GAMMASPHERE | 207 | 33 | 174 | 15.9% |
| 0rw8w2xf | Strong-field QED experiments using the BELLA PW laser dual beamlines | 205 | 95 | 110 | 46.3% |
| 3068f1p0 | Selection of high-redshift Lyman-Break Galaxies from broadband and wide photometric surveys | 203 | 79 | 124 | 38.9% |
| 57v741p8 | The Simons Observatory: A fully remote controlled calibration system with a sparse wire grid for cosmic microwave background telescopes | 199 | 150 | 49 | 75.4% |
| 85z0s9gh | New limits from microlensing on Galactic black holes in the mass range 10 M⊙ < M < 1000 M⊙ | 197 | 136 | 61 | 69.0% |
| 13045467 | Validating the galaxy and quasar catalog-level blinding scheme for the DESI 2024 analysis | 196 | 105 | 91 | 53.6% |
| 0778b8vd | Target Selection and Validation of DESI Quasars | 195 | 141 | 54 | 72.3% |
Note: Due to the evolving nature of web traffic, the data presented here should be considered approximate and subject to revision. Learn more.