Physical Sciences
Parent: Physical Sciences
eScholarship stats: Breakdown by Item for September through December, 2024
| Item | Title | Total requests | Download | View-only | %Dnld |
|---|---|---|---|---|---|
| 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 | 91 | 30 | 61 | 33.0% |
| 9hv8k11n | The Early Data Release of the Dark Energy Spectroscopic Instrument | 85 | 0 | 85 | 0.0% |
| 4v21m9h6 | THE ELEVENTH AND TWELFTH DATA RELEASES OF THE SLOAN DIGITAL SKY SURVEY: FINAL DATA FROM SDSS-III | 75 | 2 | 73 | 2.7% |
| 440232ct | Search for two neutrino double electron capture of 124Xe and 126Xe in the full exposure of the LUX detector | 73 | 2 | 71 | 2.7% |
| 70w6x41n | The BABAR detector | 73 | 58 | 15 | 79.5% |
| 8t474214 | Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Cosmological implications from two decades of spectroscopic surveys at the Apache Point Observatory | 72 | 8 | 64 | 11.1% |
| 92m6v2rq | Improving sensitivity to low-mass dark matter in LUX using a novel electrode background mitigation technique | 67 | 2 | 65 | 3.0% |
| 5nv9h19d | Cosmogenic neutron production at the Sudbury Neutrino Observatory | 59 | 2 | 57 | 3.4% |
| 6j81940n | THE NINTH DATA RELEASE OF THE SLOAN DIGITAL SKY SURVEY: FIRST SPECTROSCOPIC DATA FROM THE SDSS-III BARYON OSCILLATION SPECTROSCOPIC SURVEY | 41 | 0 | 41 | 0.0% |
| 1n37d5c5 | Target Selection and Validation of DESI Luminous Red Galaxies | 40 | 3 | 37 | 7.5% |
| 0w17c8fn | The BErkeley Lab Laser Accelerator (BELLA): A 10 GeV Laser Plasma Accelerator | 39 | 9 | 30 | 23.1% |
| 538805vh | Diagnostics, Control and Performance Parameters for the BELLA High Repetition Rate Petawatt Class Laser | 37 | 23 | 14 | 62.2% |
| 28h344th | Mu2e Conceptual Design Report | 35 | 9 | 26 | 25.7% |
| 03h3j1hg | Staging of laser-plasma accelerators | 29 | 21 | 8 | 72.4% |
| 0g466899 | The clustering of Lyman Alpha Emitting galaxies at | 29 | 2 | 27 | 6.9% |
| 6zv1v300 | Preliminary Target Selection for the DESI Luminous Red Galaxy (LRG) Sample | 29 | 13 | 16 | 44.8% |
| 02b5k6pg | Measuring Fiber Positioning Accuracy and Throughput with Fiber Dithering for the Dark Energy Spectroscopic Instrument | 28 | 5 | 23 | 17.9% |
| 3fx8c3xs | Multistage coupling of independent laser-plasma accelerators | 28 | 16 | 12 | 57.1% |
| 8br9m8hw | Deep Underground Science and Engineering Laboratory - Preliminary Design Report | 28 | 19 | 9 | 67.9% |
| 0778b8vd | Target Selection and Validation of DESI Quasars | 27 | 14 | 13 | 51.9% |
| 0v44n629 | Sloan Digital Sky Survey IV: Mapping the Milky Way, Nearby Galaxies, and the Distant Universe | 27 | 15 | 12 | 55.6% |
| 3jd3278g | Target Selection and Validation of DESI Emission Line Galaxies | 27 | 11 | 16 | 40.7% |
| 4hd2q3js | Status of the conceptual design of ALS-U | 27 | 0 | 27 | 0.0% |
| 15m6d4hm | Absolute calibration of GafChromic film for very high flux laser driven ion beams | 26 | 8 | 18 | 30.8% |
| 7k53b4mh | Design concepts for a next generation light source at LBNL | 26 | 3 | 23 | 11.5% |
| 07h356gd | Planning the Future of U.S. Particle Physics (Snowmass 2013): Chapter 8: Instrumentation Frontier | 25 | 8 | 17 | 32.0% |
| 10j633zs | A White Paper on keV sterile neutrino Dark Matter | 25 | 3 | 22 | 12.0% |
| 2km4m4pj | The Robotic Multi-Object Focal Plane System of the Dark Energy Spectroscopic Instrument (DESI) | 25 | 4 | 21 | 16.0% |
| 8qh2h744 | Preliminary Target Selection for the DESI Bright Galaxy Survey (BGS) | 25 | 13 | 12 | 52.0% |
| 9w15m5d5 | Integrated Circuit Design in US High-Energy Physics | 25 | 8 | 17 | 32.0% |
| 0hb6r7cz | Decay spectroscopy of Eu160: Quasiparticle configurations of excited states and structure of Kπ=4+ bandheads in Gd160 | 24 | 13 | 11 | 54.2% |
| 4q5441zt | The Fourteenth Data Release of the Sloan Digital Sky Survey: First Spectroscopic Data from the Extended Baryon Oscillation Spectroscopic Survey and from the Second Phase of the Apache Point Observatory Galactic Evolution Experiment | 24 | 0 | 24 | 0.0% |
| 92h0x1fh | FPGA-Based Optical Cavity Phase Stabilization for Coherent Pulse Stacking | 23 | 13 | 10 | 56.5% |
| 98w7w32d | Constraints on neutrino lifetime from the Sudbury Neutrino Observatory | 23 | 2 | 21 | 8.7% |
| 5vx8r6zf | The novel Mechanical Ventilator Milano for the COVID-19 pandemic | 22 | 3 | 19 | 13.6% |
| 730113t3 | Archetype-based Redshift Estimation for the Dark Energy Spectroscopic Instrument Survey | 22 | 3 | 19 | 13.6% |
| 9fx6c8n7 | Preliminary Target Selection for the DESI Quasar (QSO) Sample | 22 | 10 | 12 | 45.5% |
| 6ms5k3r2 | Search for nucleon decays with EXO-200 | 21 | 3 | 18 | 14.3% |
| 6zh078qk | The DESI Early Data Release white dwarf catalogue | 21 | 3 | 18 | 14.3% |
| 8xx7x681 | Characterization of the spectral phase of an intense laser at focus via ionization blueshift | 21 | 3 | 18 | 14.3% |
| 9hw4w5rg | Optimal 1D Ly α forest power spectrum estimation – III. DESI early data | 21 | 4 | 17 | 19.0% |
| 230856m0 | Design and production of the high voltage electrode grids and electron extraction region for the LZ dual-phase xenon time projection chamber | 20 | 3 | 17 | 15.0% |
| 5zj801z6 | The Supernova Type Ia Rate Evolution with SNLS | 20 | 8 | 12 | 40.0% |
| 1g06m0jb | Tests of Lorentz invariance at the Sudbury Neutrino Observatory | 19 | 2 | 17 | 10.5% |
| 84k7r6f3 | A New Light for Berkeley Lab—the Advanced Light Source Upgrade | 19 | 8 | 11 | 42.1% |
| 9772q6w0 | Electronics for the BaBar central drift chamber | 19 | 4 | 15 | 21.1% |
| 9jd644qn | High redshift LBGs from deep broadband imaging for future spectroscopic surveys | 19 | 0 | 19 | 0.0% |
| 1sf965ks | Baryon acoustic oscillations in the Lyα forest of BOSS DR11 quasars⋆ | 18 | 4 | 14 | 22.2% |
| 35b951jq | Design and vertical tests of double-quarter wave cavity prototypes for the high-luminosity LHC crab cavity system | 18 | 3 | 15 | 16.7% |
| 7qk2856p | Control of quasi-monoenergetic electron beams from laser-plasma accelerators with adjustable shock density profile | 18 | 13 | 5 | 72.2% |
Note: Due to the evolving nature of web traffic, the data presented here should be considered approximate and subject to revision. Learn more.