scispace - formally typeset
J

J. H. J. de Bruijne

Researcher at European Space Research and Technology Centre

Publications -  110
Citations -  31695

J. H. J. de Bruijne is an academic researcher from European Space Research and Technology Centre. The author has contributed to research in topics: Astrometry & Stars. The author has an hindex of 39, co-authored 100 publications receiving 27103 citations. Previous affiliations of J. H. J. de Bruijne include University of Nice Sophia Antipolis & Max Planck Society.

Papers
More filters
Journal ArticleDOI

Gaia Early Data Release 3 - Summary of the contents and survey properties (Corrigendum)

A. G. A. Brown, +461 more
Journal ArticleDOI

Gaia Data Release 1. Testing parallaxes with local Cepheids and RR Lyrae stars

G. Clementini, +637 more
TL;DR: In this article, the first parallax measurements of the primary standard candles of the cosmological distance ladder, that involve astrometry collected by Gaia during the initial 14 months of science operation, are published in Gaia Data Release 1 (DR1) as part of the Tycho-Gaia Astrometric Solution (TGAS).
Journal ArticleDOI

Gaia Data Release 1. Testing the parallaxes with local Cepheids and RR Lyrae stars

G. Clementini, +589 more
TL;DR: In this paper, the first parallax measurements of the primary standard candles of the cosmological distance ladder, that involve astrometry collected by Gaia during the initial 14 months of science operation, are published in Gaia Data Release 1 (DR1) as part of the Tycho-Gaia Astrometric Solution (TGAS).
Journal ArticleDOI

Radial velocities for the HIPPARCOS-Gaia Hundred-Thousand-Proper-Motion project

TL;DR: In this paper, the Hipparcos data were used to determine the confidence level with which the available radial velocity and its standard error, taken from the XHIP compilation catalogue, are acceptable for a 68.27% confidence level.
Journal ArticleDOI

Detecting stars, galaxies, and asteroids with Gaia

TL;DR: In this article, the authors presented a validated emulation of the on-board detection software, which has 20 free, so-called rejection parameters which govern the boundaries between stars on the one hand and sharp (high-frequency) or extended (lowfrequency) events on the other hand.