Showing 841–860 of 2,473 results
/ Date/ Name
Aug 12, 2022Methanol deuteration in high-mass protostarsAug 4, 2022The Lockman-SpReSO project. Description, target selection, observations and preliminary resultsAug 4, 2022Schrodinger's Galaxy Candidate: Puzzlingly Luminous at $z\approx17$, or Dusty/Quenched at $z\approx5$?Aug 4, 2022Developing a New Generation of Integrated Micro-Spec Far Infrared Spectrometers for the EXperiment for Cryogenic Large-Aperture Intensity Mapping (EXCLAIM)Aug 4, 2022A First Look at the Abundance Pattern -- O/H, C/O, and Ne/O -- in $z>7$ Galaxies with JWST/NIRSpecAug 3, 2022The Sparkler: Evolved High-Redshift Globular Clusters Captured by JWSTAug 2, 2022The CUBES Science CaseAug 2, 2022JWST reveals a population of ultra-red, flattened disk galaxies at 2<z<6 previously missed by HSTJul 29, 2022Testing the key role of the stellar mass-halo mass relation in galaxy merger rates and morphologies via DECODE, a novel Discrete statistical sEmi-empiriCal mODElJul 29, 2022Unveiling the Nature of Infrared Bright, Optically Dark Galaxies with Early JWST DataJul 27, 2022A New Emulated Monte Carlo Radiative Transfer Disk-Wind Model: X-Ray Accretion Disk-wind Emulator -- XRADEJul 25, 2022BASS XXII: The BASS DR2 AGN Catalog and DataJul 14, 2022Gaia Data Release 3: The first Gaia catalogue of variable AGNJul 14, 2022Compton-Thick AGN in the NuSTAR era VIII: A joint NuSTAR-XMM-Newton monitoring of the changing-look Compton-thick AGN NGC 1358Jul 13, 2022Kinematics and Mass Distributions for Non-Spherical Deprojected Sérsic Density Profiles and Applications to Multi-Component Galactic SystemsJul 12, 2022The Evolution of Lyman Alpha Emitter Line Widths from z=5.7 to z=6.6Jul 8, 2022Investigating the link between inner gravitational potential and star-formation quenching in CALIFA galaxiesJul 5, 2022Blow-Away in the Extreme Low-Mass Starburst Galaxy Pox~186Jun 29, 2022Properties of the interstellar medium in star-forming galaxies at redshifts 2 < z < 5 from the VANDELS surveyJun 27, 2022Untangling the Galaxy. IV. Empirical Constraints on Angular Momentum Evolution and Gyrochronology for Young Stars in the Field