Physical Sciences
Parent: Physical Sciences
eScholarship stats: History by Item for March through June, 2025
| Item | Title | Total requests | 2025-06 | 2025-05 | 2025-04 | 2025-03 |
|---|---|---|---|---|---|---|
| 9gm8j3mb | The construction of large-scale structure catalogs for the Dark Energy Spectroscopic Instrument | 168 | 48 | 95 | 25 | |
| 28h344th | Mu2e Conceptual Design Report | 148 | 84 | 27 | 17 | 20 |
| 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 | 142 | 61 | 31 | 25 | 25 |
| 10j633zs | A White Paper on keV sterile neutrino Dark Matter | 141 | 80 | 29 | 20 | 12 |
| 2400c76b | The Spectroscopic Data Processing Pipeline for the Dark Energy Spectroscopic Instrument | 141 | 43 | 53 | 37 | 8 |
| 70w6x41n | The BABAR detector | 124 | 41 | 35 | 22 | 26 |
| 8t474214 | Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Cosmological implications from two decades of spectroscopic surveys at the Apache Point Observatory | 117 | 46 | 22 | 21 | 28 |
| 89c1q3cb | Multiple colliding laser pulses as a basis for studying high-field high-energy physics | 109 | 63 | 16 | 11 | 19 |
| 442129hp | Synthetic spectra for Lyman-α forest analysis in the Dark Energy Spectroscopic Instrument | 108 | 46 | 21 | 24 | 17 |
| 03h3j1hg | Staging of laser-plasma accelerators | 107 | 29 | 52 | 16 | 10 |
| 538805vh | Diagnostics, Control and Performance Parameters for the BELLA High Repetition Rate Petawatt Class Laser | 106 | 45 | 30 | 20 | 11 |
| 0tc9r96f | Enhanced Isomer Population via Direct Irradiation of Solid-Density Targets Using a Compact Laser-Plasma Accelerator | 103 | 46 | 15 | 18 | 24 |
| 8qh2h744 | Preliminary Target Selection for the DESI Bright Galaxy Survey (BGS) | 97 | 45 | 29 | 11 | 12 |
| 746597bw | Comparing Compressed and Full-Modeling analyses with FOLPS: implications for DESI 2024 and beyond | 95 | 43 | 36 | 16 | |
| 6fc35504 | ELG spectroscopic systematics analysis of the DESI Data Release 1 | 94 | 41 | 53 | ||
| 5z01m0wp | Candidate strongly lensed type Ia supernovae in the Zwicky Transient Facility archive | 92 | 43 | 24 | 5 | 20 |
| 9gt3k403 | Longitudinal tapering in gas jets for increased efficiency of 10-GeV class laser plasma accelerators | 92 | 52 | 40 | ||
| 0nm3n5fp | HOD-dependent systematics in Emission Line Galaxies for the DESI 2024 BAO analysis | 91 | 37 | 36 | 18 | |
| 07h356gd | Planning the Future of U.S. Particle Physics (Snowmass 2013): Chapter 8: Instrumentation Frontier | 90 | 38 | 25 | 13 | 14 |
| 0v44n629 | Sloan Digital Sky Survey IV: Mapping the Milky Way, Nearby Galaxies, and the Distant Universe | 90 | 42 | 18 | 17 | 13 |
| 3fx8c3xs | Multistage coupling of independent laser-plasma accelerators | 87 | 46 | 23 | 14 | 4 |
| 0778b8vd | Target Selection and Validation of DESI Quasars | 86 | 27 | 21 | 25 | 13 |
| 07d801t4 | DESI 2024 III: baryon acoustic oscillations from galaxies and quasars | 86 | 31 | 34 | 21 | |
| 62g9110v | Deep Learning of Dark Energy Spectroscopic Instrument Mock Spectra to Find Damped Lyα Systems | 84 | 44 | 15 | 18 | 7 |
| 2dt5w83t | DESI 2024 VI: cosmological constraints from the measurements of baryon acoustic oscillations | 83 | 18 | 35 | 30 | |
| 4dc7x4tz | Impact of systematic redshift errors on the cross-correlation of the Lyman-α forest with quasars at small scales using DESI Early Data | 83 | 33 | 20 | 30 | |
| 3bn193b1 | The science case for an intermediate energy advanced and novel accelerator linear collider facility | 82 | 33 | 24 | 16 | 9 |
| 6zv1v300 | Preliminary Target Selection for the DESI Luminous Red Galaxy (LRG) Sample | 82 | 37 | 13 | 15 | 17 |
| 50d3k4wc | Measured Emittance Dependence on the Injection Method in Laser Plasma Accelerators | 81 | 47 | 14 | 14 | 6 |
| 1n37d5c5 | Target Selection and Validation of DESI Luminous Red Galaxies | 80 | 30 | 26 | 12 | 12 |
| 4v21m9h6 | THE ELEVENTH AND TWELFTH DATA RELEASES OF THE SLOAN DIGITAL SKY SURVEY: FINAL DATA FROM SDSS-III | 80 | 33 | 15 | 16 | 16 |
| 660639fj | Overview of the Instrumentation for the Dark Energy Spectroscopic Instrument | 80 | 33 | 24 | 12 | 11 |
| 6zk9f56d | Well Developed Deformation in Si42 | 80 | 44 | 18 | 9 | 9 |
| 5986c9r8 | Multistage Coupling of Laser-Wakefield Accelerators with Curved Plasma Channels | 79 | 44 | 16 | 6 | 13 |
| 5f17p68c | Optimal reconstruction of baryon acoustic oscillations for DESI 2024 | 79 | 24 | 38 | 17 | |
| 5vx8r6zf | The novel Mechanical Ventilator Milano for the COVID-19 pandemic | 78 | 37 | 17 | 13 | 11 |
| 2km4m4pj | The Robotic Multi-Object Focal Plane System of the Dark Energy Spectroscopic Instrument (DESI) | 77 | 35 | 23 | 9 | 10 |
| 92h0x1fh | FPGA-Based Optical Cavity Phase Stabilization for Coherent Pulse Stacking | 77 | 43 | 13 | 15 | 6 |
| 92t419x8 | Radial density profile and stability of capillary discharge plasma waveguides of lengths up to 40 cm | 77 | 24 | 20 | 12 | 21 |
| 0z21p7rc | Characterization of contaminants in the Lyman-alpha forest auto-correlation with DESI | 76 | 35 | 26 | 15 | |
| 20f4w28b | Validation of the DESI 2024 Lyman alpha forest BAL masking strategy | 76 | 48 | 20 | 8 | |
| 867528n7 | DESI 2024: reconstructing dark energy using crossing statistics with DESI DR1 BAO data | 76 | 29 | 30 | 11 | 6 |
| 8xx7x681 | Characterization of the spectral phase of an intense laser at focus via ionization blueshift | 76 | 45 | 16 | 8 | 7 |
| 9xf113n1 | A Measurement of Atmospheric Circular Polarization with POLARBEAR | 76 | 26 | 15 | 35 | |
| 0mw6677p | Powerful, pulsed, THz radiation from laser accelerated relativistic electron bunches | 75 | 24 | 12 | 2 | 37 |
| 0p92q5md | Toward the Discovery of New Elements: Production of Livermorium (Z=116) with Ti50 | 75 | 42 | 11 | 10 | 12 |
| 4b7561s0 | All-optical beamlet train generation | 75 | 54 | 6 | 5 | 10 |
| 50p9z63f | Baryon Acoustic Oscillations in the Ly-α forest of BOSS quasars | 75 | 39 | 18 | 11 | 7 |
| 1wd1z6td | Dephasing of ion beams as magnetic vortex acceleration regime transitions into a bubble-like field structure | 74 | 41 | 10 | 17 | 6 |
| 4rm62797 | Radiation pressure acceleration: The factors limiting maximum attainable ion energy | 74 | 34 | 21 | 9 | 10 |
Note: Due to the evolving nature of web traffic, the data presented here should be considered approximate and subject to revision. Learn more.