Identifying CID binaries in SDSS and in Gaia later on

Details Identifying CID binaries in SDSS and in Gaia later on Identifying CID binaries in SDSS and in Gaia later on

Oct 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aspc..338..220p&link_type=abstract

Astrometry in the Age of the Next Generation of Large Telescopes, ASP Conference Series, Vol. 338, Proceedings of a meeting held

Astronomy and Astrophysics

Astronomy

Scientific paper

The Sloan Digital Sky Survey offers the first coherent multi-wavelength astrometric programme. Measuring the position at different wavelengths makes it possible to identify binaries with similar brightness but very distinct colors, the so-called Color Induced Displacement binaries. We here present the results obtained with the third SDSS public data release and characterize briefly the spectral types of the stars involved. We then foresee how that technique could be applied to Gaia.

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