000002868 001__ 2868
000002868 005__ 20160701171712.0
000002868 0247_ $$2DOI$$a10.1017/S1743921310003637
000002868 037__ $$aASTROimport-1025
000002868 100__ $$aVallenari, A.
000002868 245__ $$aSynthetic Stellar libraries and SSP simulations in the Gaia Era
000002868 260__ $$c2010
000002868 520__ $$aThe Gaia mission will obtain accurate positions, parallaxes and proper motions for 109 object all over the sky. In addition, it will collect low resolution spectroscopy in the optical range for ~109 objects, stars, galaxies, and QSOs. Parameters of those objects are expected to be part of the final Catalog. Complete and up-to-date libraries of synthetic stellar spectra are needed to train the algorithms to classify this huge amount of data. Here we focus on the use of the synthetic libraries of spectra calculated by the Gaia community to derive grids of Single Stellar Populations as building blocks of population synthesis models. 
000002868 700__ $$a Sordo, R.
000002868 700__ $$a Tantalo, R.
000002868 700__ $$a Allard, F.
000002868 700__ $$a Blomme, R.
000002868 700__ $$a Bouret, J.-C.
000002868 700__ $$a Brott, I.
000002868 700__ $$a Fremat, Y.
000002868 700__ $$a Martayan, C.
000002868 700__ $$a Damerdji, Y.
000002868 700__ $$a Edvardsson, B.
000002868 700__ $$a Josselin, E.
000002868 700__ $$a Plez, B.
000002868 700__ $$a Kochukhov, O.
000002868 700__ $$a Kontizas, M.
000002868 700__ $$a Schweitzer, A.
000002868 700__ $$a Zorec, J.
000002868 700__ $$a Tsalmantza, P.
000002868 700__ $$a Munari, U.
000002868 700__ $$a Saguner, T.
000002868 773__ $$c444-445$$pStellar Populations - Planning for the Next Decade$$v262$$y2010
000002868 85642 $$ahttp://esoads.eso.org/abs/2010IAUS..262..444V
000002868 905__ $$apublished in
000002868 980__ $$aNONREF