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Morphology and Kinematics of the Gas in M51: How Interaction with NGC 5195 Has Molded the Structure of Its Arms |
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The Pristine Inner Galaxy Survey - VIII. Characterizing the orbital properties of the ancient, very metal-poor inner Milky Way |
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Discovery of two warm mini-Neptunes with contrasting densities orbiting the young K3V star TOI-815 |
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TOI-663: A newly discovered multi-planet system with three transiting mini-Neptunes orbiting an early M star |
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The wide-field, multiplexed, spectroscopic facility WEAVE: Survey design, overview, and simulated implementation |
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Nonlinear Wave Damping by Kelvin–Helmholtz Instability-induced Turbulence |
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High-resolution Spectroscopic Reconnaissance of a Temperate Sub-Neptune |
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Identification of the Top TESS Objects of Interest for Atmospheric Characterization of Transiting Exoplanets with JWST |
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Euclid preparation. XXXVI. Modelling the weak lensing angular power spectrum |
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The discovery space of ELT-ANDES. Stars and stellar populations |
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Euclid preparation. XXXVII. Galaxy colour selections with Euclid and ground photometry for cluster weak-lensing analyses |
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The compact multi-planet system GJ 9827 revisited with ESPRESSO★ |
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Observational Tests of Active Galactic Nuclei Feedback: An Overview of Approaches and Interpretation |
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A Perspective on the Milky Way Bulge Bar as Seen from the Neutron-capture Elements Cerium and Neodymium with APOGEE |
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Workshop summary: Kaons@CERN 2023 |
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A Very-High-Energy Gamma-Ray View of the Transient Sky |
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NGTS-28Ab: a short period transiting brown dwarf |
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The APO-K2 Catalog. II. Accurate Stellar Ages for Red Giant Branch Stars across the Milky Way |
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Long-term variability in debris transiting white dwarfs |
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Nature versus nurture: distinguishing effects from stellar processing and chemical evolution on carbon and nitrogen in red giant stars |
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The Milky Way bar pattern speed using Hercules and Gaia DR3 |
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NLTE modelling of water-rich exoplanet atmospheres. Cooling and heating rates |
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Teegarden's Star revisited. A nearby planetary system with at least three planets |
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Asymmetry in the atmosphere of the ultra-hot Jupiter WASP-76 b |
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Light new physics in B →K<SUP>(*)</SUP>ν ν ¯ ? |
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