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The homogeneity of chemical abundances in H II regions of the Magellanic Clouds |
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13 hours 39 minutes ago |
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A dense 0.1-solar-mass star in a 51-minute-orbital-period eclipsing binary |
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Automatic model-based telluric correction for the ESPRESSO data reduction software. Model description and application to radial velocity computation |
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Euclid preparation. XXI. Intermediate-redshift contaminants in the search for z > 6 galaxies within the Euclid Deep Survey |
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TOI-2196 b: Rare planet in the hot Neptune desert transiting a G-type star |
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TOI-1468: A system of two transiting planets, a super-Earth and a mini-Neptune, on opposite sides of the radius valley |
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Overview of the Instrumentation for the Dark Energy Spectroscopic Instrument |
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Particle size distributions inside and around the artificial crater produced by the Hayabusa2 impact experiment on Ryugu |
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A 4 Gyr M-dwarf Gyrochrone from CFHT/MegaPrime Monitoring of the Open Cluster M67 |
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A pristine record of outer Solar System materials from asteroid Ryugu's returned sample |
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The stellar populations of quiescent ultra-diffuse galaxies from optical to mid-infrared spectral energy distribution fitting |
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An extreme blue nugget, UV-bright starburst at z = 3.613 with 90 per cent of Lyman continuum photon escape |
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The Gaia-ESO Public Spectroscopic Survey: Motivation, implementation, GIRAFFE data processing, analysis, and final data products |
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SPECULOOS Northern Observatory: Searching for Red Worlds in the Northern Skies |
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Black hole mass and spin measurements through the relativistic precession model: XTE J1859+226 |
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A refined dynamical mass for the black hole in the X-ray transient XTE J1859+226 |
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An X-ray-quiet black hole born with a negligible kick in a massive binary within the Large Magellanic Cloud |
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The European Solar Telescope |
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