Automated Classification of Gaia Sources

Details Automated Classification of Gaia Sources Automated Classification of Gaia Sources

Aug 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aspc..394..539s&link_type=abstract

Astronomical Data Analysis Software and Systems ASP Conference Series, Vol. 394, Proceedings of the conference held 23-26 Septem

Astronomy and Astrophysics

Astronomy

3

Scientific paper

Gaia is the next generation astrometric mission from ESA, due to launch in 2011. It will survey the entire sky down to a magnitude of approximately V=20, detecting about one billion stars, or about 1% of the Galactic stellar population. Together with the stellar sample, several million galaxies, perhaps half a million quasars and many solar system objects will also be detected. No input catalogue will be used, so automated classification of detected sources is a key part of the data processing process. Here, we describe progress on the Discrete Source Classifier (DSC) which is being developed at MPIA.

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