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Massive stars in extremely metal-poor galaxies: a window into the past |
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TIC 172900988: A Transiting Circumbinary Planet Detected in One Sector of TESS Data |
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Physically Motivated Fit to Mass Surface Density Profiles Observed in Galaxies |
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The Observed Mass Distribution of Galactic Black Hole LMXBs Is Biased against Massive Black Holes |
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Wolf 503 b: Characterization of a Sub-Neptune Orbiting a Metal-poor K Dwarf |
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Euclid preparation. XII. Optimizing the photometric sample of the Euclid survey for galaxy clustering and galaxy-galaxy lensing analyses |
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An Earth-mass planet in a time of COVID-19: KMT-2020-BLG-0414Lb |
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KMT-2021-BLG-0322: Severe degeneracy between triple-lens and higher-order binary-lens interpretations |
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Molecular gas and star formation within 12 strong galactic bars observed with IRAM-30 m |
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Gas and dust from extremely metal-poor AGB stars |
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The Bias from Hydrodynamic Simulations: Mapping Baryon Physics onto Dark Matter Fields |
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Modeling the scattering polarization of the solar Ca I 4227 Å line with angle-dependent partial frequency redistribution |
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The Rossiter-McLaughlin effect revolutions: an ultra-short period planet and a warm mini-Neptune on perpendicular orbits |
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CARMENES detection of the Ca II infrared triplet and possible evidence of He I in the atmosphere of WASP-76b |
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A geometric distance to the supermassive black Hole of NGC 3783 |
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Formation of the first galaxies in the aftermath of the first supernovae |
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Dark Energy Survey year 3 results: covariance modelling and its impact on parameter estimation and quality of fit |
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