Showing 261–280 of 6,913 results
/ Date/ Name
Oct 10, 2025Euclid preparation. Cosmology Likelihood for Observables in Euclid (CLOE). 3. Inference and ForecastsOct 9, 2025The CEERS Photometric and Physical Parameter CatalogOct 9, 2025Identification of low-energy kaons in the ProtoDUNE-SP detectorOct 9, 2025Introducing SESHAT: A Tool for Object Classification from JWST CatalogsOct 7, 2025Study of few-electron backgrounds in the LUX-ZEPLIN detectorOct 7, 2025Low-energy threshold demonstration for dark matter searches in TREX-DM with an $^{37}$Ar source produced at CNA HiSPANoSOct 6, 2025Buildup, Explosion, and Untwisting of a Solar Active Region Jet Observed with Solar Orbiter, IRIS, and SDOOct 6, 2025Edge-On Disk Study (EODS) II: HCO$^+$ and CO vertical stratification in the disk surrounding SSTTau042021Oct 3, 2025A quest for sulfur-bearing refractory species. Identification of CaS in the interstellar mediumOct 2, 2025Status and future directions for direct cross-section measurements of the 13C(a,n)16O reaction for astrophysicsOct 2, 2025Constraints on sub-GeV dark matter scattering on electrons with COSINE-100Sep 30, 2025Limiting the Parameter Space for Unstable eV-scale Neutrinos Using IceCube DataSep 30, 2025Direct Measurement of Extinction in a Planet-Hosting GapSep 30, 2025Edge-On Disk Study (EODS) III: Molecular Stratification in the Flying Saucer DiskSep 29, 2025Dynamical Architectures of S-type Transiting Planets in Binaries II: A Dichotomy in Orbital Alignment of Small Planets in Close Binary SystemsSep 27, 2025ELIGANT-TN -- ELI Gamma Above Neutron Threshold: The Thermal Neutron setupSep 26, 2025GRB 250702B: Discovery of a Gamma-Ray Burst from a Black Hole Falling into a StarSep 26, 2025Galaxy Zoo: Cosmic Dawn -- morphological classifications for over 41,000 galaxies in the Euclid Deep Field North from the Hawaii Two-0 Cosmic Dawn surveySep 25, 2025Towards the Giant Radio Array for Neutrino Detection (GRAND): the GRANDProto300 and GRAND@Auger prototypesSep 23, 2025SDSS-V Black Hole Mapper: The Index Diagram as a tool to disentangle the influence of the Host Galaxy in Quasar spectra