The Gaia project: Technique, performance and status

32Citations
Citations of this article
20Readers
Mendeley users who have this article in their library.

Abstract

Gaia is a satellite mission of the ESA, aiming at absolute astrometrie measurements of about one billion stars (all stars down to 20th magnitude, with unprecedented accuracy. Additionally, magnitudes and colors will be obtained for all these stars, while radial-velocities and spectral properties will be determined only for bright objects (V < 17.5). At 15th magnitude Gaia aims at an angular accuracy of 20 microarcseconds (μ,as). This goal can only be reached if the geometry of the telescopes, the detectors, and the pointing of Gaia at each moment ("attitude") can be inferred from the Gaia measurements itself with pas accuracy. © 2008 WILEY-VCH Verlag GmbH & Co. KGaA.

Cite

CITATION STYLE

APA

Jordan, S. (2008). The Gaia project: Technique, performance and status. Astronomische Nachrichten, 329(9–10), 875–880. https://doi.org/10.1002/asna.200811065

Register to see more suggestions

Mendeley helps you to discover research relevant for your work.

Already have an account?

Save time finding and organizing research with Mendeley

Sign up for free