Abstract
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.
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References
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© 2002 Springer Science+Business Media Dordrecht
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Deveikis, V., Sperauskas, J., Vansevičius, V. (2002). Binary Star Detection with the GAIA Radial Velocity Spectrometer. In: Vansevičius, V., Kučinskas, A., Sūdžius, J. (eds) Census of the Galaxy: Challenges for Photometry and Spectrometry with GAIA. Springer, Dordrecht. https://doi.org/10.1007/978-94-010-0361-2_21
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DOI: https://doi.org/10.1007/978-94-010-0361-2_21
Publisher Name: Springer, Dordrecht
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