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Open AccessJournal ArticleDOI

Validation of the new Hipparcos reduction

F. van Leeuwen
- 01 Nov 2007 - 
- Vol. 474, Iss: 2, pp 653-664
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TLDR
In this article, a new reduction of the Hipparcos data was published, which claimed accuracies for nearly all stars brighter than magnitude Hp = 8 to be better, by up to a factor 4, than in the original catalog.
Abstract
Context. A new reduction of the astrometric data as produced by the Hipparcos mission has been published, claiming accuracies for nearly all stars brighter than magnitude Hp = 8 to be better, by up to a factor 4, than in the original catalog ue. Aims. The new Hipparcos astrometric catalogue is checked for the quality of the data and the consistency of the formal errors as well as the possible presence of error correlations. The differences with the earlier publication are explained. Methods. The internal errors are followed through the reduction proc ess, and the external errors are investigated on the basis of a comparison with radio observations of a small selection of stars, and the distribution of negative parallaxes. Error co rrelation levels are investigated and the reduction by more than a factor 10 as obtained in the new catalogue is explained. Results. The formal errors on the parallaxes for the new catalogue are confirmed. The presence of a small amount of additional noise , though unlikely, cannot be ruled out. Conclusions. The new reduction of the Hipparcos astrometric data provides an improvement by a factor 2.2 in the total weight compared to the catalogue published in 1997, and provides much improved data for a wide range of studies on stellar luminosities and local galactic kinematics.

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Journal ArticleDOI

A survey of stellar families: multiplicity of solar-type stars

TL;DR: In this article, the authors present the results of a comprehensive assessment of companions to solar-type stars, including the Sun, from the Hipparcos catalog with {pi}>40 mas, {sigma}{sub {pi/{pi}} < 0.05, 0.5 {<=} B - V {< =} 1.0 ({approx}F6-K3), and constrained by absolute magnitude and color to exclude evolved stars.
Journal ArticleDOI

Intrinsic Colors, Temperatures, and Bolometric Corrections of Pre-Main Sequence Stars

TL;DR: In this article, the intrinsic colors and temperatures of 5-30 Myr old pre-main sequence (pre-MS) stars were analyzed using optical spectra taken with the SMARTS 1.5m telescope.
Journal ArticleDOI

Intrinsic Colors, Temperatures, and Bolometric Corrections of Pre-Main Sequence Stars

TL;DR: In this article, the intrinsic colors and temperatures of 5-30 Myr old pre-main sequence (pre-MS) stars using the F0 through M9 type members of nearby, negligibly reddened groups: Eta Cha cluster, TW Hydra Association, Beta Pic Moving Group, and Tucana-Horologium Association.
References
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Book

Hipparcos, the New Reduction of the Raw Data

TL;DR: The Hipparcos mission as discussed by the authors was the first attempt to estimate the position and velocities of a single star from its photometric pass bands, which were then used to calculate the position of the satellite.
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