The transiting planet CoRoT-1b is thought to belong to the pM-class of planets, in which the thermal emission dominates in the optical wavelengths. We present a...
The secondary eclipse of the transiting exoplanet CoRoT-2b
We present a study of the light curve of the transiting exoplanet CoRoT-2b, aimed at detecting the secondary eclipse and measuring its depth. The data were...
The secondary eclipse of the transiting exoplanet CoRoT-2b (Corrigendum)
Based on observations obtained with CoRoT, a space project operated by the French Space Agency, CNES, with participation of the Science Programme of ESA, ESTEC...
The shape of oxygen abundance profiles explored with MUSE: evidence for widespread deviations from single gradients
We characterised the oxygen abundance radial distribution of a sample of 102 spiral galaxies observed with VLT/MUSE using the O3N2 calibrator. The high spatial...
The shapes of spiral arms in the S<SUP>4</SUP>G survey and their connection with stellar bars
Context. Spiral galaxies are very common in the local Universe, but their formation, evolution, and interplay with bars remain poorly understood after more than...
The sigma Orionis substellar population. VLT/FORS spectroscopy and 2MASS photometry
VLT/FORS spectroscopy and 2MASS near-infrared photometry, together with previously known data, have been used to establish the membership and the properties of...
The signature of chromospheric heating in Ca II H spectra
Context: The heating process that balances the solar chromospheric energy losses has not yet been determined. Conflicting views exist on the source of the...
The signature of high-velocity gas in the spectra of NGC 4151
The multiwavelength emission spectrum and associated velocity field of the Seyfert prototype NGC 4151 is modeled. Since the thirties NGC 4151 has been the...
The simultaneous low state spectral energy distribution of 1ES 2344+514 from radio to very high energies
Context. BL Lacertae objects are variable at all energy bands on time scales down to minutes. To construct and interpret their spectral energy distribution (SED...