International audienceThis contribution is intended as a `rough guide' to the Hipparcos Catalogue for the non-expert user. Some general aspects of the use of astrometric data are discussed as well as Hipparcos-specific applications. We discuss when and at what level one may expect systematic errors to occur in the Hipparcos Catalogue. Next we discuss the question of the interpretation of the measured parallaxes in terms of distances and luminosities of stars. What are the biases one should be aware of and how can these be corrected? When using the astrometric data to study the statistics of stars one should take the full covariance matrix of the errors on the astrometric parameters into account. We explain how to do this and discuss the spe...
A magnitude limited population of 18 808 Hipparcos stars is used to calibrate distances for 52 794 R...
International audienceA good knowledge of both accuracy and precision of the Hipparcos parallaxes is...
. The Hipparcos Input Catalogue has been compiled, over the period 1982-1991, as the definitive obse...
International audienceThis contribution is intended as a `rough guide' to the Hipparcos Catalogue fo...
The Hipparcos astrometric data will allow the determination of a great number of stellar distances. ...
Context.A new reduction of the astrometric data as produced by the Hipparcos mission has been publis...
International audienceThe principal observational characteristics of the Hipparcos Catalogue, and a ...
With the publication of the Hipparcos catalogue, astrometric data of unprecedented quality and quant...
Examples of how and when to use the Hipparcos intermediate astrometric data are presented. It is sho...
International audienceIn astrophysical applications, derived quantities like distances, absolute mag...
International audienceNew memberships, mean parallaxes and proper motions of all 9 open clusters clo...
The new reduction of the Hipparcos data presents a very significant improvement in the overall relia...
Abstract. With the publication of the Hipparcos cat-alogue, astrometric data of unprecedented qualit...
Context. A new reduction of the astrometric data as produced by the Hipparcos mission has been publi...
Vol. 1 - 5: The Hipparcos Input Catalogue. Vol. 6: Annex 1. Double and multiple stars. Vol. 7: Ann...
A magnitude limited population of 18 808 Hipparcos stars is used to calibrate distances for 52 794 R...
International audienceA good knowledge of both accuracy and precision of the Hipparcos parallaxes is...
. The Hipparcos Input Catalogue has been compiled, over the period 1982-1991, as the definitive obse...
International audienceThis contribution is intended as a `rough guide' to the Hipparcos Catalogue fo...
The Hipparcos astrometric data will allow the determination of a great number of stellar distances. ...
Context.A new reduction of the astrometric data as produced by the Hipparcos mission has been publis...
International audienceThe principal observational characteristics of the Hipparcos Catalogue, and a ...
With the publication of the Hipparcos catalogue, astrometric data of unprecedented quality and quant...
Examples of how and when to use the Hipparcos intermediate astrometric data are presented. It is sho...
International audienceIn astrophysical applications, derived quantities like distances, absolute mag...
International audienceNew memberships, mean parallaxes and proper motions of all 9 open clusters clo...
The new reduction of the Hipparcos data presents a very significant improvement in the overall relia...
Abstract. With the publication of the Hipparcos cat-alogue, astrometric data of unprecedented qualit...
Context. A new reduction of the astrometric data as produced by the Hipparcos mission has been publi...
Vol. 1 - 5: The Hipparcos Input Catalogue. Vol. 6: Annex 1. Double and multiple stars. Vol. 7: Ann...
A magnitude limited population of 18 808 Hipparcos stars is used to calibrate distances for 52 794 R...
International audienceA good knowledge of both accuracy and precision of the Hipparcos parallaxes is...
. The Hipparcos Input Catalogue has been compiled, over the period 1982-1991, as the definitive obse...