The Geneva seven-colour photometric system is successfully applied to the study of various astrophysical objects. It measures the slope of the Paschen continuum, the Balmer discontinuity, and blocking absorption due to hydrogen or metallic lines. One of its greatest strengths is its intrinsic homogeneity. A new catalogue of the available measurements was generated, 30 years after the last publication. The identifications for the individual stars were cross-checked on the basis of the Gaia and 2MASS catalogues. The high precision coordinates together with proper motions (if available) are included, for the first time, in the catalogue. Special caution was exercised with binaries and high-proper-motion stars. The catalogue includes 42 911 ent...
Context. The Carte du Ciel archive at the University of Helsinki enables us to see the sky as it was...
Stellar physical and dynamical properties are essential knowledge to understanding the structure, fo...
. The Hipparcos Input Catalogue has been compiled, over the period 1982-1991, as the definitive obse...
At the occasion of the 40th anniversary of A&A: commentary on the paper by Hog et al., 2000 entitled...
We present homogeneous, standardized UBV(RI)C photometry for over 700 nearby stars selected on the ...
Context. The uvbyβ photometric system is widely used for the study of various Galactic and extragala...
We report on a new survey of metallicities, ages, and Galactic orbits for a complete, magnitude-limi...
International audienceThe Gaia astrometric catalogue of reference stars will provide proper motions ...
Miras are fascinating stars. A kappa-mechanism in their atmosphere drives pulsations which produce c...
We present homogeneous and standardized UBV(RI)C JHK photometry for over 100 M stars selected from ...
This article has been published in Monthly Notices of the Royal Astronomical Society: Letters. © 201...
Recent CCD observations were performed in the period 1998-2004 for a large sample of visual double a...
We present the compilation of the Fifth Catalogue of Nearby Stars (CNS5), based on astrometric and p...
The Amateur Sky Survey (TASS) is a loose confederation of amateur and professional astronomers. We d...
Stellar fluxes for 531 stars in the wavelength range lambda 5500-1330A lambda are presented in the f...
Context. The Carte du Ciel archive at the University of Helsinki enables us to see the sky as it was...
Stellar physical and dynamical properties are essential knowledge to understanding the structure, fo...
. The Hipparcos Input Catalogue has been compiled, over the period 1982-1991, as the definitive obse...
At the occasion of the 40th anniversary of A&A: commentary on the paper by Hog et al., 2000 entitled...
We present homogeneous, standardized UBV(RI)C photometry for over 700 nearby stars selected on the ...
Context. The uvbyβ photometric system is widely used for the study of various Galactic and extragala...
We report on a new survey of metallicities, ages, and Galactic orbits for a complete, magnitude-limi...
International audienceThe Gaia astrometric catalogue of reference stars will provide proper motions ...
Miras are fascinating stars. A kappa-mechanism in their atmosphere drives pulsations which produce c...
We present homogeneous and standardized UBV(RI)C JHK photometry for over 100 M stars selected from ...
This article has been published in Monthly Notices of the Royal Astronomical Society: Letters. © 201...
Recent CCD observations were performed in the period 1998-2004 for a large sample of visual double a...
We present the compilation of the Fifth Catalogue of Nearby Stars (CNS5), based on astrometric and p...
The Amateur Sky Survey (TASS) is a loose confederation of amateur and professional astronomers. We d...
Stellar fluxes for 531 stars in the wavelength range lambda 5500-1330A lambda are presented in the f...
Context. The Carte du Ciel archive at the University of Helsinki enables us to see the sky as it was...
Stellar physical and dynamical properties are essential knowledge to understanding the structure, fo...
. The Hipparcos Input Catalogue has been compiled, over the period 1982-1991, as the definitive obse...