The Hipparcos astrometric data will allow the determination of a great number of stellar distances. To make a good use of their high accuracy the data have to be used with care to obtain unbiased distance estimations. We discuss in this paper the effects of the observational errors and observational selection criteria on the estimation of distances and we analyse them from a mathematical point of view. Examples are presented using Monte Carlo simulated samples. Key words: barium stars; luminosity calibration; stellar kinematics. 1. INTRODUCTION The goal of the poster presented in the Venice symposium under this title was to illustrate the problems associated with the estimation of distances using trigonometric parallaxes. These difficultie...
Context. The Hundred-Thousand-Proper-Motion (HTPM) project will determine the proper motions of ∼113...
Context. The second Gaia data release (Gaia DR2) provides precise five-parameter astrometric data (p...
Abstract. The Hipparcos solutions flagged as unreliable after the completion of the standard data pr...
International audienceThis contribution is intended as a `rough guide' to the Hipparcos Catalogue fo...
International audienceIn astrophysical applications, derived quantities like distances, absolute mag...
A magnitude limited population of 18 808 Hipparcos stars is used to calibrate distances for 52 794 R...
One of the main uses of the Hipparcos astrometric parameters is the calibration of stellar luminosit...
With the publication of the Hipparcos catalogue, astrometric data of unprecedented quality and quant...
From new geometrical parallaxes of galactic Cepheids obtained with the Hipparcos satellite a new cal...
International audienceA good knowledge of both accuracy and precision of the Hipparcos parallaxes is...
By using HIPPARCOS data (magnitudes, parallaxes, proper motions), (1) we determine new values of the...
Abstract. With the publication of the Hipparcos cat-alogue, astrometric data of unprecedented qualit...
The HR diagram luminosity calibration basically relies on trigonometric parallaxes and kinematical d...
This thesis is devoted to the validation of the stellar data which were used for the Hipparcos Input...
Context. The Hundred-Thousand-Proper-Motion (HTPM) project will determine the proper motions of ∼113...
Context. The second Gaia data release (Gaia DR2) provides precise five-parameter astrometric data (p...
Abstract. The Hipparcos solutions flagged as unreliable after the completion of the standard data pr...
International audienceThis contribution is intended as a `rough guide' to the Hipparcos Catalogue fo...
International audienceIn astrophysical applications, derived quantities like distances, absolute mag...
A magnitude limited population of 18 808 Hipparcos stars is used to calibrate distances for 52 794 R...
One of the main uses of the Hipparcos astrometric parameters is the calibration of stellar luminosit...
With the publication of the Hipparcos catalogue, astrometric data of unprecedented quality and quant...
From new geometrical parallaxes of galactic Cepheids obtained with the Hipparcos satellite a new cal...
International audienceA good knowledge of both accuracy and precision of the Hipparcos parallaxes is...
By using HIPPARCOS data (magnitudes, parallaxes, proper motions), (1) we determine new values of the...
Abstract. With the publication of the Hipparcos cat-alogue, astrometric data of unprecedented qualit...
The HR diagram luminosity calibration basically relies on trigonometric parallaxes and kinematical d...
This thesis is devoted to the validation of the stellar data which were used for the Hipparcos Input...
Context. The Hundred-Thousand-Proper-Motion (HTPM) project will determine the proper motions of ∼113...
Context. The second Gaia data release (Gaia DR2) provides precise five-parameter astrometric data (p...
Abstract. The Hipparcos solutions flagged as unreliable after the completion of the standard data pr...