Physical Sciences
Parent: Physical Sciences
eScholarship stats: Breakdown by Item for February through May, 2025
| Item | Title | Total requests | Download | View-only | %Dnld |
|---|---|---|---|---|---|
| 9gm8j3mb | The construction of large-scale structure catalogs for the Dark Energy Spectroscopic Instrument | 120 | 13 | 107 | 10.8% |
| 70w6x41n | The BABAR detector | 105 | 69 | 36 | 65.7% |
| 2400c76b | The Spectroscopic Data Processing Pipeline for the Dark Energy Spectroscopic Instrument | 104 | 61 | 43 | 58.7% |
| 8t474214 | Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Cosmological implications from two decades of spectroscopic surveys at the Apache Point Observatory | 102 | 27 | 75 | 26.5% |
| 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 | 98 | 24 | 74 | 24.5% |
| 0mw6677p | Powerful, pulsed, THz radiation from laser accelerated relativistic electron bunches | 94 | 72 | 22 | 76.6% |
| 03h3j1hg | Staging of laser-plasma accelerators | 93 | 26 | 67 | 28.0% |
| 442129hp | Synthetic spectra for Lyman-α forest analysis in the Dark Energy Spectroscopic Instrument | 92 | 35 | 57 | 38.0% |
| 28h344th | Mu2e Conceptual Design Report | 90 | 28 | 62 | 31.1% |
| 92t419x8 | Radial density profile and stability of capillary discharge plasma waveguides of lengths up to 40 cm | 76 | 6 | 70 | 7.9% |
| 538805vh | Diagnostics, Control and Performance Parameters for the BELLA High Repetition Rate Petawatt Class Laser | 75 | 41 | 34 | 54.7% |
| 89c1q3cb | Multiple colliding laser pulses as a basis for studying high-field high-energy physics | 71 | 9 | 62 | 12.7% |
| 0778b8vd | Target Selection and Validation of DESI Quasars | 69 | 30 | 39 | 43.5% |
| 4v21m9h6 | THE ELEVENTH AND TWELFTH DATA RELEASES OF THE SLOAN DIGITAL SKY SURVEY: FINAL DATA FROM SDSS-III | 68 | 4 | 64 | 5.9% |
| 3jd3278g | Target Selection and Validation of DESI Emission Line Galaxies | 67 | 18 | 49 | 26.9% |
| 8qh2h744 | Preliminary Target Selection for the DESI Bright Galaxy Survey (BGS) | 66 | 28 | 38 | 42.4% |
| 10j633zs | A White Paper on keV sterile neutrino Dark Matter | 65 | 2 | 63 | 3.1% |
| 2dt5w83t | DESI 2024 VI: cosmological constraints from the measurements of baryon acoustic oscillations | 65 | 0 | 65 | 0.0% |
| 0v44n629 | Sloan Digital Sky Survey IV: Mapping the Milky Way, Nearby Galaxies, and the Distant Universe | 64 | 11 | 53 | 17.2% |
| 6zv1v300 | Preliminary Target Selection for the DESI Luminous Red Galaxy (LRG) Sample | 64 | 28 | 36 | 43.8% |
| 1817s52c | The Atacama Cosmology Telescope DR6 and DESI: structure formation over cosmic time with a measurement of the cross-correlation of CMB lensing and luminous red galaxies | 63 | 0 | 63 | 0.0% |
| 07h356gd | Planning the Future of U.S. Particle Physics (Snowmass 2013): Chapter 8: Instrumentation Frontier | 62 | 10 | 52 | 16.1% |
| 9zb2d29s | Mitigation of DESI fiber assignment incompleteness effect on two-point clustering with small angular scale truncated estimators | 62 | 10 | 52 | 16.1% |
| 3fx8c3xs | Multistage coupling of independent laser-plasma accelerators | 61 | 32 | 29 | 52.5% |
| 4rm62797 | Radiation pressure acceleration: The factors limiting maximum attainable ion energy | 59 | 25 | 34 | 42.4% |
| 5vx8r6zf | The novel Mechanical Ventilator Milano for the COVID-19 pandemic | 58 | 6 | 52 | 10.3% |
| 867528n7 | DESI 2024: reconstructing dark energy using crossing statistics with DESI DR1 BAO data | 58 | 4 | 54 | 6.9% |
| 9n78h8r6 | Design and performance of a custom ASIC digitizer for wire chamber readout in 65 nm CMOS technology | 58 | 8 | 50 | 13.8% |
| 0tc9r96f | Enhanced Isomer Population via Direct Irradiation of Solid-Density Targets Using a Compact Laser-Plasma Accelerator | 57 | 11 | 46 | 19.3% |
| 1n37d5c5 | Target Selection and Validation of DESI Luminous Red Galaxies | 57 | 6 | 51 | 10.5% |
| 5nv9h19d | Cosmogenic neutron production at the Sudbury Neutrino Observatory | 57 | 3 | 54 | 5.3% |
| 283291nj | Overview of the SuperNova/Acceleration probe (SNAP) | 56 | 4 | 52 | 7.1% |
| 0218h457 | Dynamics and density distributions in a capillary-discharge waveguide with an embedded supersonic jet | 55 | 23 | 32 | 41.8% |
| 07d801t4 | DESI 2024 III: baryon acoustic oscillations from galaxies and quasars | 55 | 0 | 55 | 0.0% |
| 3bn193b1 | The science case for an intermediate energy advanced and novel accelerator linear collider facility | 55 | 9 | 46 | 16.4% |
| 5f17p68c | Optimal reconstruction of baryon acoustic oscillations for DESI 2024 | 55 | 7 | 48 | 12.7% |
| 0nm3n5fp | HOD-dependent systematics in Emission Line Galaxies for the DESI 2024 BAO analysis | 54 | 12 | 42 | 22.2% |
| 92h0x1fh | FPGA-Based Optical Cavity Phase Stabilization for Coherent Pulse Stacking | 54 | 25 | 29 | 46.3% |
| 9c75z2jn | DESI 2024 IV: Baryon Acoustic Oscillations from the Lyman alpha forest | 54 | 7 | 47 | 13.0% |
| 2km4m4pj | The Robotic Multi-Object Focal Plane System of the Dark Energy Spectroscopic Instrument (DESI) | 53 | 12 | 41 | 22.6% |
| 62g9110v | Deep Learning of Dark Energy Spectroscopic Instrument Mock Spectra to Find Damped Lyα Systems | 53 | 28 | 25 | 52.8% |
| 660639fj | Overview of the Instrumentation for the Dark Energy Spectroscopic Instrument | 53 | 0 | 53 | 0.0% |
| 6fc35504 | ELG spectroscopic systematics analysis of the DESI Data Release 1 | 53 | 8 | 45 | 15.1% |
| 0w17c8fn | The BErkeley Lab Laser Accelerator (BELLA): A 10 GeV Laser Plasma Accelerator | 52 | 14 | 38 | 26.9% |
| 746597bw | Comparing Compressed and Full-Modeling analyses with FOLPS: implications for DESI 2024 and beyond | 52 | 11 | 41 | 21.2% |
| 8tp707x6 | Summary report: working group 2 on "Plasma Based Acceleration Concepts" | 51 | 3 | 48 | 5.9% |
| 9hv8k11n | The Early Data Release of the Dark Energy Spectroscopic Instrument | 51 | 0 | 51 | 0.0% |
| 1sz9g710 | GeV electron beams from a centimeter-scale laser-driven plasma accelerator | 50 | 13 | 37 | 26.0% |
| 4dc7x4tz | Impact of systematic redshift errors on the cross-correlation of the Lyman-α forest with quasars at small scales using DESI Early Data | 50 | 2 | 48 | 4.0% |
| 9xf113n1 | A Measurement of Atmospheric Circular Polarization with POLARBEAR | 50 | 7 | 43 | 14.0% |
Note: Due to the evolving nature of web traffic, the data presented here should be considered approximate and subject to revision. Learn more.