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A black hole X-ray binary at ̃100 Hz: multiwavelength timing of MAXI J1820+070 with HiPERCAM and NICER |
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The Changing Rotational Light-curve Amplitude of Varuna and Evidence for a Close-in Satellite |
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Nonequilibrium ionization and ambipolar diffusion in solar magnetic flux emergence processes |
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Stellar populations of galaxies in the ALHAMBRA survey up to z ̃ 1. III. The stellar content of the quiescent galaxy population during the last 8 Gyr |
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Near-infrared spectroscopy of the Klio primitive inner-belt asteroid family |
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Interstellar Visitors: A Physical Characterization of Comet C/2019 Q4 (Borisov) with OSIRIS at the 10.4 m GTC |
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A transiting super-Earth close to the inner edge of the habitable zone of an M0 dwarf star |
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The nature of faint radio galaxies at high redshifts |
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The structural properties of classical bulges and discs from z ̃ 2 |
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Far infrared spectroscopy and other spectral and thermal properties of [Li@C60]PF6 |
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Properties of the Umbral Filament Observed in Active Region NOAA 12529 |
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NGC 7457: evidence for merger-driven cylindrical rotation in disc galaxies |
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Distribution of red clump stars does not support the X-shaped Galactic bulge |
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Lower atmosphere and pressure evolution on Pluto from ground-based stellar occultations, 1988-2016 |
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High Gas Fraction in a CO-detected Main-sequence Galaxy at z > 3 |
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Clustering properties of TGSS radio sources |
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The kinematics of local thick discs do not support an accretion origin⋆ |
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A New Einstein Cross Gravitational Lens of a Lyman-break Galaxy |
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The CARMENES search for exoplanets around M dwarfs. Period search in Hα, Na I D, and Ca II IRT lines |
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