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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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An Enigmatic High Excitation Nebula in IC 1613 Dwarf Galaxy |
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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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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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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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Infrared Spectral Fingerprint of Neutral and Charged Endo- and Exohedral Metallofullerenes |
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Beyond the 3rd moment: a practical study of using lensing convergence CDFs for cosmology with DES Y3 |
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Extreme photometric and polarimetric variability of blazar S4 0954+65 at its maximum optical and γ-ray brightness levels |
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KMT-2021-BLG-1547Lb: Giant microlensing planet detected through a signal deformed due to source binarity |
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Void BAO measurements on quasars from eBOSS |
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Detection of optical emission from the supernova remnant G7.7-3.7 |
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TOI-4600 b and c: Two Long-period Giant Planets Orbiting an Early K Dwarf |
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Fossil group origins. XIII. A paradigm shift: Fossil groups as isolated structures rather than relics of the ancient Universe |
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Long-term trends in albedo as seen from a lunar observatory |
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A method to deconvolve stellar profiles. The non-rotating line utilizing Gaussian sum approximation |
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Magnetic Activity Evolution of Solar-like Stars. I. S <SUB>ph</SUB>-Age Relation Derived from Kepler Observations |
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