000002234 001__ 2234
000002234 005__ 20160701171701.0
000002234 0247_ $$2DOI$$a10.1088/1742-6596/328/1/012006
000002234 037__ $$aASTROimport-391
000002234 100__ $$aSordo, R.
000002234 245__ $$aStellar libraries for Gaia
000002234 260__ $$c2011
000002234 520__ $$aGaia will observe up to a billion stellar sources. Automated algorithms are under development to derive the atmospheric parameters of all observed spectra, from low resolution optical spectra alone or in synergy with high resolution spectra in the near-IR Ca II triplet region. To do so, a large database of state-of-the-art stellar libraries has been produced for the Gaia community, computed using different codes optimized for specific purposes. The choice to use different spectral codes in different regions of the H-R diagram raises the problem of the coherence of the different spectra, specifically in the transition zones. We present a comparison between the libraries from the point of view of spectra simulations for training the Gaia algorithms. We also present the implementation of these libraries into a Simple Stellar Population code. 
000002234 700__ $$a Vallenari, A.
000002234 700__ $$a Tantalo, R.
000002234 700__ $$a Liu, C.
000002234 700__ $$a Smith, K.
000002234 700__ $$a Allard, F.
000002234 700__ $$a Blomme, R.
000002234 700__ $$a Bouret, J.-C.
000002234 700__ $$a Brott, I.
000002234 700__ $$a de Laverny, P.
000002234 700__ $$a Edvardsson, B.
000002234 700__ $$a Frémat, Y.
000002234 700__ $$a Heber, U.
000002234 700__ $$a Josselin, E.
000002234 700__ $$a Kochukhov, O.
000002234 700__ $$a Korn, A.
000002234 700__ $$a Lanzafame, A.
000002234 700__ $$a Martayan, C.
000002234 700__ $$a Martins, F.
000002234 700__ $$a Plez, B.
000002234 700__ $$a Schweitzer, A.
000002234 700__ $$a Thévenin, F.
000002234 700__ $$a Zorec, J.
000002234 773__ $$c012006$$i1$$pJournal of Physics Conference Series$$v328$$y2011
000002234 85642 $$ahttp://esoads.eso.org/abs/2011JPhCS.328a2006S
000002234 905__ $$apublished in
000002234 980__ $$aREFERD