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The 2023 Outburst of the Gaia Alerted EXor Gaia23bab |
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INSPIRE: INvestigating Stellar Populations In RElics - IX. KiDS J0842 + 0059: the first fully confirmed relic beyond the local Universe |
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A targeted search for binary white dwarf pulsars using Gaia and WISE |
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A new way to measure the distance to NGC1052-DF2 |
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The Mini-SiTian Array: First-two-year Operation |
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The Complete Spitzer Survey of Stellar Structure in Galaxies (CS<SUP>4</SUP>G) |
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Euclid: IV. The NISP Calibration Unit |
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Detection of Methane in the Closest Extreme Metal-poor T Dwarf WISEA J181006.18‑101000.5 |
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Search for new Galactic Wolf–Rayet stars using Gaia DR3: I. Candidate selection and the follow-up of the bright sample |
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The GAPS Programme at TNG: LXVII. Detection of water and preliminary characterisation of the atmospheres of the two hot Jupiters: KELT-8 b and KELT-23 Ab |
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Gaia20bdk – New FU Ori-type star in the Sh 2-301 star-forming region |
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Reduced atomic models for large-scale computations: Fe XIII near-infrared lines |
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It is not σ<SUB>8</SUB>: constraining the non-linear matter power spectrum with the Dark Energy Survey Year-5 supernova sample |
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Intervening nuclear obscuration changing the X-ray look of the z ≈ 6 quasi-stellar object CFHQS J164121+375520 |
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The wide binary frequency of metal-poor stars |
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The Galaxy Activity, Torus, and Outflow Survey (GATOS). VII. The 20–214 μm Imaging Atlas of Active Galactic Nuclei Using SOFIA |
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The Galaxy Activity, Torus, and Outflow Survey (GATOS): VI. Black hole mass estimation using machine learning |
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DALI sensitivity to streaming axion dark matter |
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Requirements on the gain calibration for LiteBIRD polarisation data with blind component separation |
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The Intrinsic Flattening of Galaxy Disks |
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KMT-2021-BLG-0284, KMT-2022-BLG-2480, and KMT-2024-BLG-0412: Three microlensing events involving two lens masses and two source stars |
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Expanding the Ultracompacts: Gravitational-wave-driven Mass Transfer in the Shortest-period Binaries with Accretion Disks |
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Copacabana: a probabilistic membership assignment method for galaxy clusters |
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