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Accuracy of the radial velocities and efficiency of the spectroscopic binary detection with the GAIA radial velocity spectrometer (RVS) is evaluated by employing the observed spectra (Cenarro et al., 2001) and simulated GAIA observations. Evaluation is performed in the magnitude range V =10-17 by applying the cross-correlation method. This revised version was published online in July 2006 with corrections to the Cover Date.  相似文献   
2.
We present a software package developed for modelling of the GAIA photometric observations. The modelling procedure is very flexible and fully controlled via the parameter file. Therefore, configuration of the GAIA telescopes and photometric systems, as well as the object samples under investigation, can be adjusted easily. This revised version was published online in July 2006 with corrections to the Cover Date.  相似文献   
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