Showing 1–20 of 410 results
/ Date/ Name
Apr 16, 2026The nEXO Radioassay ProgramMar 13, 2026Qubit syndrome measurements with a high fidelity Rb-Cs Rydberg gateFeb 27, 2026Design of a high voltage delivery system for noble liquid time projection chambersDec 11, 2025Characterization of CRYO ASIC for charge readout in the nEXO experimentNov 17, 2025Search for Double Beta Decays of $^{134}$Xe with EXO-200 Phase IIOct 16, 2025Measurement of $C\!P$ asymmetry in $D^0 \to K^0_{\rm S} K^0_{\rm S}$ decays with Run 3 dataAug 11, 2025Ultra-pure Nickel for Structural Components of Low-Radioactivity InstrumentsAug 8, 2025A D/H Ratio Consistent with Earth's Water in Halley-type Comet 12P from ALMA HDO MappingJul 31, 2025Simulation-based inference for Precision Neutrino Physics through Neural Monte Carlo tuningJun 27, 2025Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark MatterApr 24, 2025Measurement of the Parity-Violating Asymmetry in the N to $Δ$ Transition at Low $Q^2$Apr 21, 2025Ultra-sensitive radon assay using an electrostatic chamber in a recirculating systemNov 15, 2024BICEP/Keck XIX: Extremely Thin Composite Polymer Vacuum Windows for BICEP and Other High Throughput Millimeter Wave TelescopesSep 3, 2024Development of the 220/270 GHz Receiver of BICEP ArrayAug 15, 2024A universal neutral-atom quantum computer with individual optical addressing and non-destructive readoutJul 30, 2024Mitigating calibration errors from mutual coupling with time-domain filtering of 21 cm cosmological radio observationsJun 29, 2024Imaging of single barium atoms in a second matrix site in solid xenon for barium tagging in a $^{136}$Xe double beta decay experimentJun 27, 2024Isotropy of cosmic rays beyond $10^{20}$ eV favors their heavy mass compositionJun 27, 2024Mass composition of ultra-high energy cosmic rays from distribution of their arrival directions with the Telescope ArrayJun 12, 2024Investigating Mutual Coupling in the Hydrogen Epoch of Reionization Array and Mitigating its Effects on the 21-cm Power Spectrum