000002555 001__ 2555
000002555 005__ 20160701171707.0
000002555 037__ $$aASTROimport-712
000002555 100__ $$aMartayan, C.
000002555 245__ $$aThe Gaia satellite: a tool for Emission Line Stars and Hot Stars
000002555 260__ $$c2008
000002555 520__ $$aThe Gaia satellite will be launched at the end of 2011. It will observe at least 1 billion stars, and among them several million emission line stars and hot stars. Gaia will provide parallaxes for each star and spectra for stars till V magnitude equal to 17. After a general description of Gaia, we present the codes and methods, which are currently developed by our team. They will provide automatically the astrophysical parameters and spectral classification for the hot and emission line stars in the Milky Way and other close local group galaxies such as the Magellanic Clouds. 
000002555 700__ $$a Frémat, Y.
000002555 700__ $$a Blomme, R.
000002555 700__ $$a Jonckheere, A.
000002555 700__ $$a Borges, M.
000002555 700__ $$a de Batz, B.
000002555 700__ $$a Leroy, B.
000002555 700__ $$a Sordo, R.
000002555 700__ $$a Bouret, J.-C.
000002555 700__ $$a Martins, F.
000002555 700__ $$a Zorec, J.
000002555 700__ $$a Neiner, C.
000002555 700__ $$a Nazé, Y.
000002555 700__ $$a Alecian, E.
000002555 700__ $$a Floquet, M.
000002555 700__ $$a Hubert, A.-M.
000002555 700__ $$a Briot, D.
000002555 700__ $$a Miroshnichenko, A.
000002555 700__ $$a Kolka, I.
000002555 700__ $$a Stee, P.
000002555 700__ $$a Lanz, T.
000002555 700__ $$a Meynet, G.
000002555 773__ $$c499$$pSF2A-2008$$y2008
000002555 85642 $$ahttp://esoads.eso.org/abs/2008sf2a.conf..499M
000002555 905__ $$apublished in
000002555 980__ $$aNONREF