Physical Sciences

Parent: Physical Sciences

eScholarship stats: Breakdown by Item for April through July, 2026

ItemTitleTotal requestsDownloadView-only%Dnld
9j80t4m1The 16th Data Release of the Sloan Digital Sky Surveys: First Release from the APOGEE-2 Southern Survey and Full Release of eBOSS Spectra95009500.0%
1946q35dDESI 2024: Constraints on physics-focused aspects of dark energy using DESI DR1 BAO data54235518765.5%
6dn8z4sgCosmological constraints from the cross-correlation of DESI Luminous Red Galaxies with CMB lensing from Planck PR4 and ACT DR648035112973.1%
867528n7DESI 2024: reconstructing dark energy using crossing statistics with DESI DR1 BAO data4807140914.8%
6p44s2tvAdiabatic matching of particle bunches in a plasma-based accelerator in the presence of ion motion4553876885.1%
2dt5w83tDESI 2024 VI: cosmological constraints from the measurements of baryon acoustic oscillations42210431824.6%
1kp7z8trLaser-heated capillary discharge plasma waveguides for electron acceleration to 8 GeV41726515263.5%
8xn4v0s5Dynamical dark energy in light of the DESI DR2 baryonic acoustic oscillations measurements41426714764.5%
10j633zsA White Paper on keV sterile neutrino Dark Matter39720219550.9%
2km4m4pjThe Robotic Multi-Object Focal Plane System of the Dark Energy Spectroscopic Instrument (DESI)37122914261.7%
0rw8w2xfStrong-field QED experiments using the BELLA PW laser dual beamlines33214618644.0%
6fc35504ELG spectroscopic systematics analysis of the DESI Data Release 132822110767.4%
9zb2d29sMitigation of DESI fiber assignment incompleteness effect on two-point clustering with small angular scale truncated estimators3252368972.6%
8gg3z5b3DESI 2024 V: Full-Shape galaxy clustering from galaxies and quasars32417914555.2%
3813v2tsStabilization and control of persistent current magnets using variable inductance32314917446.1%
0tc9r96fEnhanced Isomer Population via Direct Irradiation of Solid-Density Targets Using a Compact Laser-Plasma Accelerator3212239869.5%
2px009hqAchievement of Target Gain Larger than Unity in an Inertial Fusion Experiment31411120335.4%
7nv6c95nConstraining primordial non-Gaussianity with DESI 2024 LRG and QSO samples3142387675.8%
0p92q5mdToward the Discovery of New Elements: Production of Livermorium (Z=116) with Ti5031112418739.9%
5mm917mqSpontaneous fission of the odd-Z isotope Db25530418312160.2%
28z4k02hConstraints on neutrino physics from DESI DR2 BAO and DR1 full shape30111918239.5%
5502f0rkA comparison between ShapeFit compression and Full-Modelling method with PyBird for DESI 2024 and beyond28616312357.0%
28h344thMu2e Conceptual Design Report28115212954.1%
8t474214Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Cosmological implications from two decades of spectroscopic surveys at the Apache Point Observatory28117810363.3%
538805vhDiagnostics, Control and Performance Parameters for the BELLA High Repetition Rate Petawatt Class Laser2802077373.9%
91g0w6f1The 13th Data Release of the Sloan Digital Sky Survey: First Spectroscopic Data from the SDSS-IV Survey Mapping Nearby Galaxies at Apache Point Observatory27910817138.7%
6zh078qkThe DESI Early Data Release white dwarf catalogue2741888668.6%
0fv331g6DESI DR2 results. II. Measurements of baryon acoustic oscillations and cosmological constraints27302730.0%
3fx8c3xsMultistage coupling of independent laser-plasma accelerators26915311656.9%
4338r7m1DESI Emission-line Galaxies: Clustering Dependence on Stellar Mass and [O II] Luminosity2681927671.6%
9x16p56fEnhancing DESI DR1 full-shape analyses using HOD-informed priors2672076077.5%
67q6j3gfCosmological implications of DESI DR2 BAO measurements in light of the latest ACT DR6 CMB data2656719825.3%
70w6x41nThe BABAR detector2561678965.2%
85z0s9ghNew limits from microlensing on Galactic black holes in the mass range 10 M⊙ < M < 1000 M⊙2561619562.9%
0778b8vdTarget Selection and Validation of DESI Quasars2511925976.5%
8qh2h744Preliminary Target Selection for the DESI Bright Galaxy Survey (BGS)24912812151.4%
13045467Validating the galaxy and quasar catalog-level blinding scheme for the DESI 2024 analysis2471588964.0%
79p4v28zGeV electron beams from a cm-scale accelerator2435119221.0%
33t0027tTHE SDSS-IV EXTENDED BARYON OSCILLATION SPECTROSCOPIC SURVEY: QUASAR TARGET SELECTION2411865577.2%
9gm8j3mbThe construction of large-scale structure catalogs for the Dark Energy Spectroscopic Instrument2411429958.9%
0xh894czOnline charge measurement for petawatt laser-driven ion acceleration2391667369.5%
1hz6q3jxComparative study of active plasma lenses in high-quality electron accelerator transport lines2371617667.9%
07h356gdPlanning the Future of U.S. Particle Physics (Snowmass 2013): Chapter 8: Instrumentation Frontier23512511053.2%
0z2063j6A joint analysis of 3D clustering and galaxy × CMB-lensing cross-correlations with DESI DR1 galaxies2351587767.2%
5217c2bmLaser-heated capillary discharge waveguides as tunable structures for laser-plasma acceleration23412311152.6%
3jd3278gTarget Selection and Validation of DESI Emission Line Galaxies2331686572.1%
67f7s5bkDESI 2024 II: sample definitions, characteristics, and two-point clustering statistics2291567368.1%
95g853gvThe clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample22912410554.1%
1ch809d5Modified gravity constraints from the full shape modeling of clustering measurements from DESI 202422811311549.6%
978149tjValidation of the DESI 2024 Lyα forest BAO analysis using synthetic datasets2281735575.9%

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