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Quasar Microlensing Statistics and Flux-ratio Anomalies in Lens Models |
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Characterizing the ELG luminosity functions in the nearby Universe |
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Cosmology and fundamental physics with the ELT-ANDES spectrograph |
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Confirmation of a Sub-Saturn-size Transiting Exoplanet Orbiting a G Dwarf: TOI-1194 b and a Very Low Mass Companion Star: TOI-1251 B from TESS |
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A post-merger enhancement only in star-forming Type 2 Seyfert galaxies: the deep learning view |
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MANCHA3D Code: Multipurpose Advanced Nonideal MHD Code for High-Resolution Simulations in Astrophysics |
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An Enigmatic High Excitation Nebula in IC 1613 Dwarf Galaxy |
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Orbit of the Patroclus–Menoetius Binary System and Predictions for the 2024/2025 Mutual Events Season |
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Detection of an intranight optical hard lag with colour variability in blazar PKS 0735+178 |
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Constraining the reflective properties of WASP-178 b using CHEOPS photometry |
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On the dust properties of the UV galaxies in the redshift range z 0.6-1.2 |
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The three hundred project: mapping the matter distribution in galaxy clusters via deep learning from multiview simulated observations |
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Experimental measurement of the quality factor of a Fabry-Pérot open-cavity axion haloscope |
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The Hubble tension survey: A statistical analysis of the 2012-2022 measurements |
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TIC 378898110: A bright, short-period AM CVn binary in TESS |
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The black widow pulsar J1641+8049 in the optical, radio, and X-rays |
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Gaia Focused Product Release: Asteroid orbital solution. Properties and assessment |
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No random transits in CHEOPS observations of HD 139139 |
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Performance of the joint LST-1 and MAGIC observations evaluated with Crab Nebula data |
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A plausible link between dynamically unsettled molecular gas and the radio jet in NGC 6328 |
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JWST Constraints on the UV Luminosity Density at Cosmic Dawn: Implications for 21 cm Cosmology |
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CHEOPS and TESS view of the ultra-short-period super-Earth TOI-561 b |
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CHEX-MATE: A non-parametric deep learning technique to deproject and deconvolve galaxy cluster X-ray temperature profiles |
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Scaling slowly rotating asteroids with stellar occultations |
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The <SUP>12</SUP>C/<SUP>13</SUP>C isotopic ratio at the dawn of chemical evolution |
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