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Neutron star mass estimates from gamma-ray eclipses in spider millisecond pulsar binaries |
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Identification of tidal features in deep optical galaxy images with convolutional neural networks |
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Galaxy interactions are the dominant trigger for local type 2 quasars |
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Observations of two superfast rotator NEAs: 2021 NY<SUB>1</SUB> and 2022 AB |
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Another shipment of six short-period giant planets from TESS |
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Overview of the DESI Milky Way Survey |
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Confirmation of Color-dependent Centroid Shift Measured After 1.8 Years with HST |
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Temporal Structures in Electron Spectra and Charge Sign Effects in Galactic Cosmic Rays |
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The miniJPAS survey: AGN and host galaxy coevolution of X-ray-selected sources |
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Dark Energy Survey Year 3 results: Constraints on extensions to Λ CDM with weak lensing and galaxy clustering |
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The SAMI-Fornax Dwarfs Survey - III. Evolution of [α/Fe] in dwarfs, from Galaxy Clusters to the Local Group |
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Estimating the longitudinal magnetic field in the chromosphere of quiet-Sun magnetic concentrations |
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joshspeagle/dynesty: v2.1.0 |
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Improved High-resolution Fast Imager |
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DAHe white dwarfs from the DESI Survey |
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CEERS Key Paper. IV. A Triality in the Nature of HST-dark Galaxies |
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The Fornax3D project: Environmental effects on the assembly of dynamically cold disks in Fornax cluster galaxies |
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Bright extragalactic ALMA redshift survey (BEARS) III: detailed study of emission lines from 71 Herschel targets |
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Expectations of the Size Evolution of Massive Galaxies at 3 ≤ z ≤ 6 from the TNG50 Simulation: The CEERS/JWST View |
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WEAVE-StePS: A stellar population survey using WEAVE at WHT |
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A super-Earth and a mini-Neptune near the 2:1 MMR straddling the radius valley around the nearby mid-M dwarf TOI-2096 |
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Forming intracluster gas in a galaxy protocluster at a redshift of 2.16 |
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First BISTRO Observations of the Dark Cloud Taurus L1495A-B10: The Role of the Magnetic Field in the Earliest Stages of Low-mass Star Formation |
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TOI-2525 b and c: A Pair of Massive Warm Giant Planets with Strong Transit Timing Variations Revealed by TESS |
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CEERS Key Paper. II. A First Look at the Resolved Host Properties of AGN at 3 < z < 5 with JWST |
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