Stellar Galactic Population Characterization using Gaia Photometry

Details Stellar Galactic Population Characterization using Gaia Photometry Stellar Galactic Population Characterization using Gaia Photometry

Jan 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005esasp.576..155c&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

Astrophysics

Gaia, Photometry, Filter Definition, Astrophysical Parameters

Scientific paper

The spectroscopic features to be measured, their dependence as a function of Teff , log g or [M/H] for the various types of stars leading us to the design of the medium passbands, central wavelength and their blue and red limits are described. The design particularly accounts for the scientific key targets for the study of the origin and history of our Galaxy. This paper focusses on the GenevaBarcelona medium-band photometric system.

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