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Colour and infall time distributions of satellite galaxies in simulated Milky-Way analogues |
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Prospects for future studies using deep imaging: analysis of individual Galactic cirrus filaments |
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The Lockman-SpReSO project. Description, target selection, observations, and catalogue preparation |
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Asteroids' reflectance from Gaia DR3: Artificial reddening at near-UV wavelengths |
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CHRONOSTAR - II. Kinematic age and substructure of the Scorpius-Centaurus OB2 association |
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The Dawes Review 10: The impact of deep learning for the analysis of galaxy surveys |
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Photosynthetic Fluorescence from Earthlike Planets around Sunlike and Cool Stars |
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Vortex Motions in the Solar Atmosphere |
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55 Cancri e's occultation captured with CHEOPS |
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Formation of the Mg II h and k Polarization Profiles in a Solar Plage Model and Their Suitability to Infer Magnetic Fields |
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First detection of the outer edge of an AGN accretion disc: very fast multiband optical variability of NGC 4395 with GTC/HiPERCAM and LT/IO:O |
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QUIJOTE scientific results - VIII. Diffuse polarized foregrounds from component separation with QUIJOTE-MFI |
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New physics searches at kaon and hyperon factories |
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Samples returned from the asteroid Ryugu are similar to Ivuna-type carbonaceous meteorites |
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ERGO-ML I: inferring the assembly histories of IllustrisTNG galaxies from integral observable properties via invertible neural networks |
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Extragalactic Magnetism with SOFIA (SALSA Legacy Program): The Magnetic Fields in the Multiphase Interstellar Medium of the Antennae Galaxies |
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Moving groups across Galactocentric radius with Gaia DR3 |
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The galaxy size to halo spin relation of disc galaxies in cosmological hydrodynamical simulations |
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Keck spectroscopy of the coma cluster ultra-diffuse galaxy Y358: dynamical mass in a wider context |
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Optical spectroscopy of blazars for the Cherenkov Telescope Array - II |
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Two decades of optical timing of the shortest-period binary star system HM Cancri |
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Toward measuring supermassive black hole masses with interferometric observations of the dust continuum |
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Consistent lensing and clustering in a low-S<SUB>8</SUB> Universe with BOSS, DES Year 3, HSC Year 1, and KiDS-1000 |
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STRIDES: automated uniform models for 30 quadruply imaged quasars |
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