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Ultra-bright CO and [{\rm{C}}\,{\rm{I}}] Emission in a Lensed z = 2.04 Submillimeter Galaxy with Extreme Molecular Gas Properties |
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Stokes inversion based on convolutional neural networks |
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Temporal changes of the flare activity of Proxima Centauri |
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The Pristine survey - V. A bright star sample observed with SOPHIE |
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Erratum: Erratum to: Search for a new scalar resonance decaying to a pair of Z bosons in proton-proton collisions at √{s} = 13 TeV |
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Physical Properties of a Coma-analog Protocluster at z = 6.5 |
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TOI-150: A Transiting Hot Jupiter in the TESS Southern CVZ |
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Understanding the evolution of close white dwarf binaries |
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Inference of magnetic field strength and density from damped transverse coronal waves |
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Polarization of changing-look quasars |
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Gaia-assisted selection of a quasar reddened by dust in an extremely strong damped Lyman-α absorber at z = 2.226 |
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Optically Faint Massive Balmer Break Galaxies at z > 3 in the CANDELS/GOODS Fields |
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Qatar Exoplanet Survey: Qatar-8b, 9b, and 10b—A Hot Saturn and Two Hot Jupiters |
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Measurement of the extragalactic background light using MAGIC and Fermi-LAT gamma-ray observations of blazars up to z = 1 |
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Torus model properties of an ultra-hard X-ray selected sample of Seyfert galaxies |
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Proxima Centauri b is not a transiting exoplanet |
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Physical properties of PHA 2014 JO25 from a worldwide observational campaign |
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Primeval very low-mass stars and brown dwarfs - VI. Population properties of metal-poor degenerate brown dwarfs |
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Stellar spectral models compared with empirical data |
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Chemical analysis of CH stars - III. Atmospheric parameters and elemental abundances |
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The VLT-FLAMES Tarantula Survey. XXXI. Radial velocities and multiplicity constraints of red supergiant stars in 30 Doradus |
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The XMM-Newton/HST View of the Obscuring Outflow in the Seyfert Galaxy Mrk 335 Observed at Extremely Low X-Ray Flux |
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QUIJOTE scientific results - III. Microwave spectrum of intensity and polarization in the Taurus Molecular Cloud complex and L1527 |
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HD 219666 b: a hot-Neptune from TESS Sector 1 |
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Diagnostic potential of the Ca II 8542 Å line for solar filaments |
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