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Near optimal angular quadratures for polarised radiative transfer |
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Hot Exoplanet Atmospheres Resolved with Transit Spectroscopy (HEARTS). III. Atmospheric structure of the misaligned ultra-hot Jupiter WASP-121b |
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Lowly Polarized Light from a Highly Magnetized Jet of GRB 190114C |
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Erratum: The Herschel Bright Sources (HerBS): sample definition and SCUBA-2 observations |
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MEGARA-GTC stellar spectral library: I |
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Discovery of a pre-cataclysmic binary with unusual chromaticity of the eclipsed white dwarf by the GPX survey |
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The Pristine survey XI: the FORS2 sample |
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LHS 1815b: The First Thick-disk Planet Detected by TESS |
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Characterization of M-stars in the LMC in the JWST era |
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Early Optical Observations of Gamma-Ray Bursts Compared with Their Gamma- and X-Ray Characteristics Using a MASTER Global Network of Robotic Telescopes from Lomonosov Moscow State University |
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TOI-132 b: A short-period planet in the Neptune desert transiting a V = 11.3 G-type star<SUP>★</SUP> |
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VVV WIN 1733-3349: a low extinction window to probe the far side of the Milky Way bulge |
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NOEMA redshift measurements of bright Herschel galaxies |
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Multiplicity of the red supergiant population in the young massive cluster NGC 330 |
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Modeling the Strongest Silicate Emission Features of Local Type 1 AGNs |
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Arp 70: an interacting galaxy with extreme outflows |
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New Hard-TeV Extreme Blazars Detected with the MAGIC Telescopes |
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Tracking Downflows from the Chromosphere to the Photosphere in a Solar Arch Filament System |
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Analysis in the visible range of NASA Lucy mission targets: Eurybates, Polymele, Orus and Donaldjohanson. |
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The Formation of a 70 M<SUB>☉</SUB> Black Hole at High Metallicity |
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Stellar atmospheric parameters of FGK-type stars from high-resolution optical and near-infrared CARMENES spectra |
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Mass determinations of the three mini-Neptunes transiting TOI-125 |
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The Role of Environment in Galaxy Evolution in the SERVS Survey. I. Density Maps and Cluster Candidates |
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The young massive SMC cluster NGC 330 seen by MUSE. I. Observations and stellar content |
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Two-dimensional simulations of coronal rain dynamics. I. Model consisting of a vertical magnetic field and an unbounded atmosphere |
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