Gaia Data Reduction Tasks for Double and Multiple Stars

Details Gaia Data Reduction Tasks for Double and Multiple Stars Gaia Data Reduction Tasks for Double and Multiple Stars

Jan 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005esasp.576..557a&link_type=abstract

"Proceedings of the Gaia Symposium "The Three-Dimensional Universe with Gaia" (ESA SP-576). Held at the Observatoire de Paris-Me

Astronomy and Astrophysics

Astronomy

3

Scientific paper

As a result of the different instruments on-board Gaia and their various spatial or time resolutions, millions of Double and Multiple Stars (DMS) will be detected, of almost every kind. Accordingly, the data processing of DMS will undoubtedly be complex. This processing can be described in broad categories: resolved doubles and multiple stars, astrometric, spectroscopic, photometric or eclipsing binaries and classification task; in total, not less than 32 algorithms may be needed, which also call for adapted simulations.

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