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On the interpolation of model atmospheres and high-resolution synthetic stellar spectra |
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The puzzling merging cluster Abell 1914: new insights from the kinematics of member galaxies |
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The multiwavelength polarization of Cygnus X-1 |
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Searching for the signatures of terrestrial planets in F-, G-type main-sequence stars |
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No temperature fluctuations in the giant H II region H 1013 |
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Planck intermediate results. V. Pressure profiles of galaxy clusters from the Sunyaev-Zeldovich effect |
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Planck intermediate results. VIII. Filaments between interacting clusters |
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GTC OSIRIS z-band imaging of Y dwarfs |
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Oxygen Abundances in Nearby FGK Stars and the Galactic Chemical Evolution of the Local Disk and Halo |
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Virgo cluster and field dwarf ellipticals in 3D - I. On the variety of stellar kinematic and line-strength properties |
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Multiwavelength spectral evolution during the 2011 outburst of the very faint X-ray transient Swift J1357.2-0933 |
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A complex state transition from the black hole candidate Swift J1753.5-0127 |
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The QUIJOTE-CMB experiment: studying the polarisation of the galactic and cosmological microwave emissions |
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Organizational transformation into the operational phase of the GTC |
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Design of the J-PAS and J-PLUS filter systems |
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Properties of convective motions in facular regions |
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Resolving the Internal Magnetic Structure of the Solar Network |
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The Hanle Effect of Lyα in a Magnetohydrodynamic Model of the Solar Transition Region |
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Observation and modelling of main-sequence star chromospheres - XIX. FIES and FEROS observations of dM1 stars |
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Exploring the α-enhancement of metal-poor planet-hosting stars. The Kepler and HARPS samples |
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Anomalous Circular Polarization Profiles in the He I 1083.0 nm Multiplet from Solar Spicules |
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Infrared Study of Fullerene Planetary Nebulae |
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Simultaneous Multi-Wavelength Observations of Magnetic Activity in Ultracool Dwarfs. III. X-ray, Radio, and Hα Activity Trends in M and L dwarfs |
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An HST/WFPC2 survey of bright young clusters in M 31. IV. Age and mass estimates |
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Specific star formation and the relation to stellar mass from 0 < z < 2 as seen in the far-infrared at 70 and 160 μm |
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