Showing 461–480 of 3,595 results
/ Date/ Name
Jul 14, 2024Supernova Pointing Capabilities of DUNEJul 13, 2024Photocathode characterisation for robust PICOSEC Micromegas precise-timing detectorsJul 11, 2024Centrality dependence of Lévy-stable two-pion Bose-Einstein correlations in $\sqrt{s_{_{NN}}}=200$ GeV Au$+$Au collisionsJul 10, 2024Few-electron highly charged muonic Ar atoms verified by electronic $K$ x raysJul 8, 2024Improved limit on neutrinoless double beta decay of $^{100}$Mo from AMoRE-IJul 5, 2024Spectroscopy of deeply bound orbitals in neutron-rich Ca isotopesJul 4, 2024Kappa-tail technique: Modeling and application to Solar Energetic Particles observed by Parker Solar ProbeJul 3, 2024Upper Limit on the Photoproduction Cross Section of the Spin-Exotic $π_1(1600)$Jul 3, 2024Measurement of the branching fraction of the decay $J/ψ\to p \bar{p} η$Jul 1, 2024Measurement of the integrated luminosity of data samples collected during 2019-2022 by the Belle II experimentJun 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 28, 2024High-energy spectra of LTT 1445A and GJ 486 reveal flares and activityJun 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 27, 2024The Space Coronagraph Optical Bench (SCoOB): 5. End-to-end simulations of polarization aberrationsJun 26, 2024Rapid Mid-Infrared Spectral-Timing with JWST. I. The prototypical black hole X-ray Binary GRS 1915+105 during a MIR-bright and X-ray-obscured stateJun 26, 2024Playing with FIRE: A Galactic Feedback-Halting Experiment Challenges Star Formation Rate TheoriesJun 23, 2024Measurement of the $\mathrm{{}^{12}C}(e,e')$ cross sections at $Q^2=0.8\,\mathrm{GeV}^2/c^2$Jun 23, 2024Discovery of a cold giant planet and mass measurement of a hot super-Earth in the multi-planetary system WASP-132Jun 22, 2024XMM-Newton Ultra Narrow Deep Field survey II: X-ray spectral analysis of the brightest AGN population