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TOI-519 b: A short-period substellar object around an M dwarf validated using multicolour photometry and phase curve analysis |
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Vetting of 384 TESS Objects of Interest with TRICERATOPS and Statistical Validation of 12 Planet Candidates |
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A statistical study of plasmoids associated with a post-CME current sheet |
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Exploring the Galactic Warp through Asymmetries in the Kinematics of the Galactic Disk |
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Wide binaries in planetary nebulae with Gaia DR2 |
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Probing Jet Launching in Neutron Star X-Ray Binaries: The Variable and Polarized Jet of SAX J1808.4-3658 |
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WASP-127b: a misaligned planet with a partly cloudy atmosphere and tenuous sodium signature seen by ESPRESSO |
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The CARMENES search for exoplanets around M dwarfs. LP 714-47 b (TOI 442.01): populating the Neptune desert |
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The EDGE-CALIFA survey: exploring the role of molecular gas on galaxy star formation quenching |
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Separation between RR Lyrae and type II Cepheids and their importance for a distance determination: the case of omega Cen |
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Evolutionary and pulsation properties of Type II Cepheids |
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Mapping the stellar age of the Milky Way bulge with the VVV. III. High-resolution reddening map |
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The kinematics of young and old stellar populations in nuclear rings of MUSE TIMER galaxies |
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Perturbation theory for modeling galaxy bias: Validation with simulations of the Dark Energy Survey |
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A Systematic Search of Zwicky Transient Facility Data for Ultracompact Binary LISA-detectable Gravitational-wave Sources |
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Coronal Heating by MHD Waves |
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Homogeneity in the early chemical evolution of the Sextans dwarf spheroidal galaxy |
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HADES RV programme with HARPS-N at TNG. XII. The abundance signature of M dwarf stars with planets |
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Broadband transmission spectroscopy of HD 209458b with ESPRESSO: evidence for Na, TiO, or both |
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Variations in color and reflectance on the surface of asteroid (101955) Bennu |
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Distribution of star formation in galactic bars as seen with Hα and stacked GALEX UV imaging |
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Galactic cirri in deep optical imaging |
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Spectroscopic classification of a complete sample of astrometrically-selected quasar candidates using Gaia DR2 |
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Euclid preparation. X. The Euclid photometric-redshift challenge |
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Charm physics confronts high-p<SUB>T</SUB> lepton tails |
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Hace 4 days 4 hours |
