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TESS and ESPRESSO discover a super-Earth and a mini-Neptune orbiting the K-dwarf TOI-238* |
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The first measurements of carbon isotopic ratios in post-RGB stars: SZ Mon and DF Cyg |
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Revealing the characteristics of the dark GRB 150309A: Dust extinguished or high-z? |
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The dynamical state of bars in cluster dwarf galaxies: the cases of NGC 4483 and NGC 4516 |
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Hydrogenated amorphous carbon grains as an alternative carrier of the 9-13 μm plateau feature in the fullerene planetary nebula Tc 1 |
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A dynamic view of V Hydrae. Monitoring of a spectroscopic-binary AGB star with an alkaline jet |
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Two fluid dynamics in solar prominences |
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Masses, revised radii, and a third planet candidate in the 'Inverted' planetary system around TOI-1266 |
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The CARMENES search for exoplanets around M dwarfs. Telluric absorption corrected high S/N optical and near-infrared template spectra of 382 M dwarf stars |
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Stellar spectral-type (mass) dependence of the dearth of close-in planets around fast-rotating stars. Architecture of Kepler confirmed single-exoplanet systems compared to star-planet evolution models |
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The GW Vir Instability Strip in Light of New Observations of PG 1159 Stars: Discovery of Pulsations in the Central Star of A72 and Variability of RX J0122.9-7521 |
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The orbital period of the recurrent nova V2487 Oph revealed |
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A compact multi-planet system transiting HIP 29442 (TOI-469) discovered by TESS and ESPRESSO. Radial velocities lead to the detection of transits with low signal-to-noise ratio |
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TESS Spots a Super-puff: The Remarkably Low Density of TOI-1420b |
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Stellar metallicity from optical and UV spectral indices: Test case for WEAVE-StePS |
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Borderline hyperbolic comet C/2021 O3 (PANSTARRS) was fading as it approached the Sun |
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Opacity for realistic 3D MHD simulations of cool stellar atmospheres |
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Synchronous Rotation in the (136199) Eris-Dysnomia System |
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CO<SUB>2</SUB> as the main parent source of atomic oxygen in comet C/2017 K2 (Pan-STARRS) |
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Uncertainty-aware blob detection with an application to integrated-light stellar population recoveries |
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Physical properties of NEOs derived from their phase curves |
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The Carbon Star DY Persei May Be a Cool R Coronae Borealis Variable |
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