The Radial Velocity Experiment (RAVE): A 1 Million Star Survey for Exploring the Formation History of the Galaxy

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Scientific paper

The Radial Velocity Experiment (RAVE) is an ambitious all-sky spectroscopic survey to measure radial velocities and stellar atmosphere parameters (temperature, surface gravity) and abundances of up to one million stars using the 6dF multi-object spectrograph on the 1.2-m UK Schmidt Telescope of the Anglo-Australian Observatory (AAO). RAVE is a multi-national endeavour involving scientists from 10 countries. Since the operation of RAVE started in April 2003, almost 400 000 spectra have been taken in the Ca-triplet region (8410-8790 Å) for southern hemisphere stars in the magnitude range 9 < I < 13 at a resolution of R=7500. The radial velocities measured in this survey are accurate to 2-3 kilometers per second. RAVE has meanwhile published two data releases, a third data release is scheduled for early 2010. Science applications of RAVE include the identification of substructure in the Milky Way and to derive constraints on the gravitational potential of our Galaxy.

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