Bibcode
                                    
                            Katz, D.; Cropper, M.; Meynadier, F.; Jean-Antoine, A.; Allende Prieto, C.; Baker, S.; Benson, K.; Berthier, J.; Bigot, L.; Blomme, R.; Boudreault, S.; Chemin, L.; Crifo, F.; Damerdji, Y.; David, M.; David, P.; Delle Luche, C.; Dolding, C.; Frémat, Y.; Gerbier, N.; Gerssen, J.; Gómez, A.; Gosset, E.; Guerrier, A.; Guy, L.; Hall, D.; Hestroffer, D.; Huckle, H.; Jasniewicz, G.; Ludwig, H.-G.; Martayan, C.; Morel, T.; Nguyen, A.-T.; Ocvirk, P.; Parr, C.; Royer, F.; Sartoretti, P.; Seabroke, G.; Simon, E.; Smith, M.; Soubiran, C.; Steinmetz, M.; Thévenin, F.; Turon, C.; Udry, S.; Veltz, L.; Viala, Y.
    Referencia bibliográfica
                                    EAS Publications Series, Volume 45, 2011, pp.189-194
Fecha de publicación:
    
                        2
            
                        2011
            
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                                    0
                            Número de citas referidas
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                            Descripción
                                    During the five years of the mission, the Gaia spectrograph, the Radial
Velocity Spectrometer (RVS) will repeatedly survey the celestial sphere
down to magnitude V ~ 17-18. This talk presents: (i) the system which is
currently developed within the Gaia Data Processing and Analysis
Consortium (DPAC) to reduce and calibrate the spectra and to derive the
radial and rotational velocities, (ii) the RVS expected performances and
(iii) scientific returns.