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QUIJOTE Scientific Results - XVII. Studying the anomalous microwave emission in the Andromeda Galaxy with QUIJOTE-MFI |
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Probing cosmic inflation with the LiteBIRD cosmic microwave background polarization survey |
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Author Correction: A super-massive Neptune-sized planet |
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On the Magnetic Nature of Quiet-Sun Chromospheric Grains |
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Long-term trends in albedo as seen from a lunar observatory |
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Correction to: Strong CO absorption features in massive ETGs |
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A sub-Neptune transiting the young field star HD 18599 at 40 pc |
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Stellar metallicity gradients of Local Group dwarf galaxies (Corrigendum) |
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Detection of the Irregular Shape of the Southern Limb of Menoetius from Observations of the 2017-2018 Patroclus-Menoetius Mutual Events |
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Observational and numerical characterization of a recurrent arc-shaped front propagating along a coronal fan |
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A comprehensive study of the opposition effect on 15 NEOs |
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Dust Emission in Galaxies at Millimeter Wavelengths: Cooling of star forming regions in NGC6946 |
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Individual dynamical masses of DENIS J063001.4-184014AB reveal a likely young brown dwarf triple |
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Self-interacting dark matter and the delay of supermassive black hole growth |
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Modeling the contamination of Bennu and Ryugu through catastrophic disruption of their precursors |
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Spectral characterisation of 14 V-type candidate asteroids from the MOVIS catalogue |
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Erratum: MUSEQuBES: Calibrating the redshifts of Lyα emitters using stacked circumgalactic medium absorption profiles |
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The CARMENES search for exoplanets around M dwarfs. Photospheric parameters of target stars from high-resolution spectroscopy. II. Simultaneous multi-wavelength range modeling of activity insensitive lines (Corrigendum) |
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An Image of the Dust Sublimation Region in the Nucleus of NGC 1068 |
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Growth and disruption in the Lyra complex |
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Distribution and spectrophotometric classification of basaltic asteroids |
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Mapping Galaxy Clusters in the Distant Universe |
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Radial Velocities in the Outermost Disk toward the Anticenter |
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Chemical and Kinematic Analysis of CN-strong Metal-poor Field Stars in LAMOST DR3 |
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Impact of Exoplanet Science in the Early Twenty-First Century |
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Hace 1 year 4 months |
