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Magnetic fields in M dwarfs from the CARMENES survey |
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Stokes inversion based on convolutional neural networks |
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An old, metal-poor globular cluster in Sextans A and the metallicity floor of globular cluster systems |
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FCC-ee: The Lepton Collider. Future Circular Collider Conceptual Design Report Volume 2 |
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FCC Physics Opportunities |
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Spectropolarimetric analysis of an active region filament. I. Magnetic and dynamical properties from single component inversions |
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The Fornax Deep Survey (FDS) with VST. VI. Optical properties of the dwarf galaxies in the Fornax cluster |
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Can a negative-mass cosmology explain dark matter and dark energy? |
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VLT/FLAMES high-resolution chemical abundances in Sculptor: a textbook dwarf spheroidal galaxy |
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MONOS: Multiplicity Of Northern O-type Spectroscopic systems. I. Project description and spectral classifications and visual multiplicity of previously known objects |
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A Hot Saturn Orbiting an Oscillating Late Subgiant Discovered by TESS |
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The Main Sequence at z ∼ 1.3 Contains a Sizable Fraction of Galaxies with Compact Star Formation Sizes: A New Population of Early Post-starbursts? |
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A near-infrared study of the multiphase outflow in the type-2 quasar J1509+0434 |
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Assembly bias evidence in close galaxy pairs |
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Prospects for measurements with strange hadrons at LHCb |
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Spectral Distortions of the CMB as a Probe of Inflation, Recombination, Structure Formation and Particle Physics |
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Stellar Physics and Galactic Archaeology using Asteroseismology in the 2020's |
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Reduction of the maximum mass-loss rate of OH/IR stars due to unnoticed binary interaction |
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Lower atmosphere and pressure evolution on Pluto from ground-based stellar occultations, 1988-2016 |
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Polarization of changing-look quasars |
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The CARMENES search for exoplanets around M dwarfs. Different roads to radii and masses of the target stars |
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The CORALIE survey for southern extrasolar planets. XVIII. Three new massive planets and two low-mass brown dwarfs at greater than 5 AU separation |
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The Fornax 3D project: Thick disks in a cluster environment |
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The evolution of luminous red nova AT 2017jfs in NGC 4470 |
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ALMA Reveals Potential Evidence for Spiral Arms, Bars, and Rings in High-redshift Submillimeter Galaxies |
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