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The resolved size and structure of hot dust in the immediate vicinity of AGN |
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3 weeks 5 days ago |
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The Typical Massive Quiescent Galaxy at z ∼ 3 is a Post-starburst |
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Extended Hα over compact far-infrared continuum in dusty submillimeter galaxies. Insights into dust distributions and star-formation rates at z ∼ 2 |
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TESS Spots a Hot Jupiter with an Inner Transiting Neptune |
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RedDots: a temperate 1.5 Earth-mass planet candidate in a compact multiterrestrial planet system around GJ 1061 |
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The Continuing Search for Evidence of Tidal Orbital Decay of Hot Jupiters |
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The Magnetic Sensitivity of the Resonance and Subordinate Lines of Mg II in the Solar Chromosphere |
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The Hubble Space Telescope UV Legacy Survey of Galactic Globular Clusters. XX. Ages of Single and Multiple Stellar Populations in Seven Bulge Globular Clusters |
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The frequency of gaseous debris discs around white dwarfs |
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The First Ultracompact Roche Lobe-Filling Hot Subdwarf Binary |
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Candidate Brown-dwarf Microlensing Events with Very Short Timescales and Small Angular Einstein Radii |
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Two Ultra-faint Milky Way Stellar Systems Discovered in Early Data from the DECam Local Volume Exploration Survey |
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Serendipitous Discovery of a Physical Binary Quasar at z = 1.76 |
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The X-shooter Spectral Library (XSL): Data release 2 |
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Evolution of Stokes V area asymmetry related to a quiet Sun cancellation observed with GRIS/IFU |
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Stellar Characterization of M Dwarfs from the APOGEE Survey: A Calibrator Sample for M-dwarf Metallicities |
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The Tarantula Massive Binary Monitoring. III. Atmosphere analysis of double-lined spectroscopic systems |
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Peculiar emission line spectra of core extremely red BOSS quasars at z̃2-3: orientation and/or evolution? |
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Trojans in the Solar Neighborhood |
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The Great Markarian 421 Flare of 2010 February: Multiwavelength Variability and Correlation Studies |
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GJ 1252 b: A 1.2 R<SUB>⊕</SUB> Planet Transiting an M3 Dwarf at 20.4 pc |
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New constraints on the structure of the nuclear stellar cluster of the Milky Way from star counts and MIR imaging |
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The Properties of the Interstellar Medium of Galaxies across Time as Traced by the Neutral Atomic Carbon [C i] |
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An empirical, Bayesian approach to modelling crop yield: Maize in USA |
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A physically motivated definition for the size of galaxies in an era of ultradeep imaging |
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