Showing 301–320 of 7,744 results
/ Date/ Name
Sep 22, 2025Modeling Scintillation Photon Transport and Reconstruction Algorithms for the Time-of-Flight Detector in the T2K Neutrino ExperimentSep 19, 2025A New Way to Discover Strong Gravitational Lenses: Pair-wise Spectroscopic Search from DESI DR1Sep 18, 2025Low-energy nuclear recoil calibration of the LUX-ZEPLIN experiment with a photoneutron sourceSep 18, 2025Detection and characterisation of a 106-day transiting Jupiter : TOI-2449 b / NGTS-36 bSep 18, 2025A high geometric albedo and small size of the Haumea cluster member (24835) 1995 SM55 from a stellar occultation and photometric observationsSep 18, 2025DESI DR1 Ly$α$ forest: 3D full-shape analysis and cosmological constraintsSep 18, 2025Stratified wind from a super-Eddington X-ray binary is slower than expectedSep 15, 2025A high fraction of close massive binary stars at low metallicitySep 11, 2025Discovery and Analysis of Afterglows from Poorly Localised GRBs with the Gravitational-wave Optical Transient Observer (GOTO) All-sky SurveySep 11, 2025Progress toward a demonstration of high contrast imaging at ultraviolet wavelengthsSep 11, 2025Current problems of studying relativistic dissociation of light nuclei in nuclear emulsionSep 10, 2025Time-Dependent Modeling of the Sub-Hour Spectral Evolution During the 2013 Outburst of Mrk 421Sep 9, 2025Spatial resolution studies with the BabyIAXO Micromegas prototypeSep 9, 2025Measurement of muon neutrino induced charged current interactions without charged pions in the final state using a new T2K off-axis near detector WAGASCI-BabyMINDSep 9, 2025SN 2022xlp: The second-known well-observed, intermediate-luminosity Iax supernovaSep 9, 2025Towards mono-energetic virtual $ν$ beam cross-section measurements: A feasibility study of $ν$-Ar interaction analysis with DUNE-PRISMSep 8, 2025Active galactic nuclei-heated dust revealed in "little red dots"Sep 8, 2025First Production of Skipper-CCD Modules for the DAMIC-M ExperimentSep 8, 2025PRIMER & JADES reveal an abundance of massive quiescent galaxies at 2 < z < 5Sep 8, 2025Understanding JWST water spectra: what can thermochemical models tell us about the (cold) water in protoplanetary disks?