Showing 61–80 of 358 results
/ Date/ Name
Oct 2, 2024JWST Observations of Young protoStars (JOYS). Overview of gaseous molecular emission and absorption in low-mass protostarsAug 30, 2024Two-neutrino double electron capture of $^{124}$Xe in the first LUX-ZEPLIN exposureAug 20, 2024EWOCS-II: X-ray properties of the Wolf-Rayet stars in the young Galactic super star cluster Westerlund 1Aug 10, 2024Mass determination of two Jupiter-sized planets orbiting slightly evolved stars: TOI-2420 b and TOI-2485 bJul 30, 2024Obliquity Constraints for the Extremely Eccentric Sub-Saturn Kepler-1656 bJun 19, 2024Local structure maturation in high entropy oxide (Mg,Co,Ni,Cu,Zn)1-x(Cr,Mn)xO thin filmsJun 4, 2024Probing the Scalar WIMP-Pion Coupling with the first LUX-ZEPLIN dataMay 23, 2024The Data Acquisition System of the LZ Dark Matter Detector: FADRMay 21, 2024Gliese 12 b, A Temperate Earth-sized Planet at 12 Parsecs Discovered with TESS and CHEOPSMay 16, 2024KiDS-1000 and DES-Y1 combined: Cosmology from peak count statisticsMay 2, 2024The Design, Implementation, and Performance of the LZ Calibration SystemsApr 26, 2024Constraints On Covariant WIMP-Nucleon Effective Field Theory Interactions from the First Science Run of the LUX-ZEPLIN ExperimentMar 8, 2024The Wide-field Spectroscopic Telescope (WST) Science White PaperMar 7, 2024Emission lines due to ionizing radiation from a compact object in the remnant of Supernova 1987AFeb 14, 2024New constraints on ultraheavy dark matter from the LZ experimentDec 14, 2023EWOCS-I: The catalog of X-ray sources in Westerlund 1 from the Extended Westerlund 1 and 2 Open Clusters SurveyDec 4, 2023First Constraints on WIMP-Nucleon Effective Field Theory Couplings in an Extended Energy Region From LUX-ZEPLINNov 28, 2023Constraining Stellar Rotation at the Zero-Age Main Sequence with TESSNov 14, 2023The Gaia-ESO Survey: 3D dynamics of young groups and clusters from GES and Gaia EDR3Nov 5, 2023Measuring the CMB primordial B-modes with Bolometric Interferometry