Author/Authors :
Antonella Vallenari، نويسنده , , Rosanna Sordo and Emanuela Chiosi، نويسنده , , Rosaria Tantalo، نويسنده , , France Allard، نويسنده , , Ronny Blomme، نويسنده , , Jean-Claud Bouret، نويسنده , , Ines Brott، نويسنده , , Yves Fremat، نويسنده , , Christophe Martayan، نويسنده , , Yassine Damerdji، نويسنده , , Bengt Edvardsson، نويسنده , , Eric Josselin، نويسنده , , Bertrand Plez، نويسنده , , Oleg Kochukhov، نويسنده , , Mary Kontizas، نويسنده , , Andreas Sch، نويسنده ,
Abstract :
The Gaia mission will obtain accurate positions, parallaxes and proper motions for 109 object all over the sky. In addition, it will collect low resolution spectroscopy in the optical range for ∼ 109 objects, stars, galaxies, and QSOs. Parameters of those objects are expected to be part of the final Catalog. Complete and up-to-date libraries of synthetic stellar spectra are needed to train the algorithms to classify this huge amount of data. Here we focus on the use of the synthetic libraries of spectra calculated by the Gaia community to derive grids of Single Stellar Populations as building blocks of population synthesis models.
