Engineering
Parent: Physical Sciences
eScholarship stats: Breakdown by Item for April through July, 2026
| Item | Title | Total requests | Download | View-only | %Dnld |
|---|---|---|---|---|---|
| 9zp8p7nm | FCC-hh: The Hadron Collider | 876 | 570 | 306 | 65.1% |
| 1n1690zv | Progress on HL-LHC Nb<sub>3</sub>Sn Magnets | 756 | 153 | 603 | 20.2% |
| 8br9m8hw | Deep Underground Science and Engineering Laboratory - Preliminary Design Report | 619 | 379 | 240 | 61.2% |
| 1946q35d | DESI 2024: Constraints on physics-focused aspects of dark energy using DESI DR1 BAO data | 542 | 355 | 187 | 65.5% |
| 0g69b4vb | SEARCHES FOR TIME-DEPENDENT NEUTRINO SOURCES WITH ICECUBE DATA FROM 2008 TO 2012 | 501 | 57 | 444 | 11.4% |
| 11v2v9vc | Generating mock galaxy catalogues for flux-limited samples like the DESI Bright Galaxy Survey | 488 | 354 | 134 | 72.5% |
| 6dn8z4sg | Cosmological constraints from the cross-correlation of DESI Luminous Red Galaxies with CMB lensing from Planck PR4 and ACT DR6 | 480 | 351 | 129 | 73.1% |
| 867528n7 | DESI 2024: reconstructing dark energy using crossing statistics with DESI DR1 BAO data | 480 | 71 | 409 | 14.8% |
| 5823k370 | The LUX-ZEPLIN (LZ) experiment | 443 | 308 | 135 | 69.5% |
| 9b14n7g1 | The ATLAS Experiment at the CERN Large Hadron Collider | 424 | 286 | 138 | 67.5% |
| 1xp428p2 | HE-LHC: The High-Energy Large Hadron Collider | 422 | 291 | 131 | 69.0% |
| 2dt5w83t | DESI 2024 VI: cosmological constraints from the measurements of baryon acoustic oscillations | 422 | 104 | 318 | 24.6% |
| 8xn4v0s5 | Dynamical dark energy in light of the DESI DR2 baryonic acoustic oscillations measurements | 414 | 267 | 147 | 64.5% |
| 5w02m2h9 | The ABC130 barrel module prototyping programme for the ATLAS strip tracker | 395 | 282 | 113 | 71.4% |
| 2km4m4pj | The Robotic Multi-Object Focal Plane System of the Dark Energy Spectroscopic Instrument (DESI) | 371 | 229 | 142 | 61.7% |
| 4g2920kn | Operation and performance of the ATLAS semiconductor tracker in LHC Run 2 | 368 | 0 | 368 | 0.0% |
| 44q234z2 | Fabrication and Test of C3a: A Six-Layer Subscale Canted $\cos \theta$ Dipole Magnet Using High-Temperature Superconducting corc Wires | 361 | 269 | 92 | 74.5% |
| 7xn8533z | Superconducting ECR ion source: From 24-28 GHz SECRAL to 45 GHz fourth generation ECR | 357 | 233 | 124 | 65.3% |
| 37s69828 | Berkeley MET5: Engineering precision and stability for 8 nm resolution EUV lithography | 356 | 189 | 167 | 53.1% |
| 78f398d8 | Search for Neutrino Doublets and Triplets Using 11.4 yr of IceCube Data | 352 | 223 | 129 | 63.4% |
| 7fs8w6m8 | The 4D Camera: An 87 kHz Direct Electron Detector for Scanning/Transmission Electron Microscopy | 347 | 203 | 144 | 58.5% |
| 06w3q8dx | ANTARES and IceCube Combined Search for Neutrino Point-like and Extended Sources in the Southern Sky | 342 | 185 | 157 | 54.1% |
| 94k948wv | A Review of the Mechanical Properties of Materials Used in Nb3Sn Magnets for Particle Accelerators | 337 | 182 | 155 | 54.0% |
| 00g7374m | Combined search for neutrinos from dark matter self-annihilation in the Galactic Center with ANTARES and IceCube | 333 | 212 | 121 | 63.7% |
| 3fh431f8 | All-sky Neutrino Point-source Search with IceCube Combined Track and Cascade Data | 329 | 223 | 106 | 67.8% |
| 6fc35504 | ELG spectroscopic systematics analysis of the DESI Data Release 1 | 328 | 221 | 107 | 67.4% |
| 9zb2d29s | Mitigation of DESI fiber assignment incompleteness effect on two-point clustering with small angular scale truncated estimators | 325 | 236 | 89 | 72.6% |
| 8gg3z5b3 | DESI 2024 V: Full-Shape galaxy clustering from galaxies and quasars | 324 | 179 | 145 | 55.2% |
| 3813v2ts | Stabilization and control of persistent current magnets using variable inductance | 323 | 149 | 174 | 46.1% |
| 12q424wz | Search for Continuous and Transient Neutrino Emission Associated with IceCube’s Highest-energy Tracks: An 11 yr Analysis | 322 | 256 | 66 | 79.5% |
| 2ks5b3d4 | Spatial and temporal evaluations of the liquid argon purity in ProtoDUNE-SP | 318 | 212 | 106 | 66.7% |
| 31t007fw | IceCube-Gen2: the window to the extreme Universe | 317 | 224 | 93 | 70.7% |
| 5350s08s | First search for dark matter annihilations in the Earth with the IceCube detector | 313 | 192 | 121 | 61.3% |
| 9vp4840m | Production and integration of the ATLAS Insertable B-Layer | 313 | 163 | 150 | 52.1% |
| 0p92q5md | Toward the Discovery of New Elements: Production of Livermorium (Z=116) with Ti50 | 311 | 124 | 187 | 39.9% |
| 7c5386wx | Conceptual Design of ILC Damping Ring Wiggler Straight Vacuum System | 310 | 243 | 67 | 78.4% |
| 3bt7p471 | New Technologies for Discovery | 308 | 54 | 254 | 17.5% |
| 8m8301pk | Constraining High-energy Neutrino Emission from Supernovae with IceCube | 308 | 221 | 87 | 71.8% |
| 60h5f1d3 | Supernova pointing capabilities of DUNE | 307 | 65 | 242 | 21.2% |
| 3255929v | Updated cosmological constraints on axion dark energy with DESI | 305 | 159 | 146 | 52.1% |
| 5mm917mq | Spontaneous fission of the odd-Z isotope Db255 | 304 | 183 | 121 | 60.2% |
| 8718k9vm | Deep Underground Neutrino Experiment (DUNE) Near Detector Conceptual Design Report | 304 | 50 | 254 | 16.4% |
| 9jf276tx | Jet energy measurement with the ATLAS detector in proton-proton collisions at | 304 | 229 | 75 | 75.3% |
| 05g0d59g | Multimessenger Gamma-Ray and Neutrino Coincidence Alerts Using HAWC and IceCube Subthreshold Data | 303 | 175 | 128 | 57.8% |
| 9hh8w4jf | Time-integrated Southern-sky Neutrino Source Searches with 10 yr of IceCube Starting-track Events at Energies Down to 1 TeV | 303 | 145 | 158 | 47.9% |
| 2nk3m7d2 | Search for quantum gravity using astrophysical neutrino flavour with IceCube | 302 | 233 | 69 | 77.2% |
| 61v754fp | Solar fusion cross sections. II. The pp chain and CNO cycles | 299 | 62 | 237 | 20.7% |
| 18w717zp | Search for sub-TeV Neutrino Emission from Novae with IceCube-DeepCore | 295 | 181 | 114 | 61.4% |
| 127666wd | Search for annihilating dark matter in the Sun with 3 years of IceCube data | 294 | 172 | 122 | 58.5% |
| 0km96259 | An Initial Look at the Magnetic Design of a 150 mm Aperture High-Temperature Superconducting Magnet With a Dipole Field of 8 to 10 T | 293 | 200 | 93 | 68.3% |
Note: Due to the evolving nature of web traffic, the data presented here should be considered approximate and subject to revision. Learn more.