Showing 121–140 of 7,941 results
/ Date/ Name
Feb 20, 2026Investigating the role of mergers in galaxy assembly in the early Universe (z > 5)Feb 20, 2026dfcosmic: A Python package for cosmic ray removalFeb 18, 2026Measurement of the Muon Flux at the Sanford Underground Research Facility with the LUX-ZEPLIN Dark Matter DetectorFeb 17, 2026The COHERENT Experiment: 2026 UpdateFeb 16, 2026Barium Stars Across the Milky Way: Probing Their Origins via the GALAH SurveyFeb 13, 2026LHAASO observation of Mrk 421 during 2021 March - 2024 March: a comprehensive VHE catalog of multi-timescale outbursts and its time average behaviorFeb 12, 2026Parker Solar Probe observations of solar energetic particle (SEP) events with inverse velocity arrival (IVA) featuresFeb 11, 2026Evidence for Shallow Nebular Attenuation Curves and Patchy Dust Geometry at z~2 with Pa-beta/H-alpha Measurements from JWST-MegaScience Medium Band PhotometryFeb 11, 20263D insights into SN 1987A: ALMA observations compared to hydrodynamical explosion simulationsFeb 10, 2026Investigating the Nested Structure of the Outflow from the Low Luminosity Protostar IRAS 16253-2429 using JWST and ALMAFeb 6, 2026Non-spherical BUFFALOs: a weak lensing view of the Frontier Field clusters and associated systematicsFeb 6, 2026First results from the E302 efficiency$\unicode{x2013}$instability experiment at the FACET-II facilityFeb 3, 2026The Tarantula massive binary monitoring VII. The nature of the eccentric O+BH binary candidate VFTS 812Feb 3, 2026Production of GEM-like structures for cryogenic applications, using laser-cutting techniquesFeb 2, 2026Mitigating half-wave plate systematics at the map-making level: calibration requirements for LiteBIRDFeb 2, 2026PRISMS. UNCOVER-26185, a metal-poor SFG at z=10.05 with no evidence for a X-ray-luminous AGNFeb 2, 2026PRISMS. U37126, a very blue, ISM-naked starburst at z=10.255 with nearly 100% Lyman continuum escape fractionFeb 2, 2026Pilots and Other Predictable Elements of the Starlink Ku-Band DownlinkJan 29, 2026The Little Blue and Red Dots Rosetta Stones: Non-Gaussian broad lines, hot dust, and X-ray weaknessJan 28, 2026Performance of the Particle-Identification Silicon-Telescope Array Coupled with the VAMOS++ Magnetic Spectrometer