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Galactic Archeology with RAVE and TGAS

Published online by Cambridge University Press:  02 August 2018

Matthias Steinmetz Open the ORCID record for Matthias Steinmetz [Opens in a new window]  and
the RAVE collaboration
Matthias Steinmetz
Affiliation:
Leibniz-Institut für Astrophysik Potsdam (AIP), An der Sternwarte 16, 14482 Potsdam, Germany, email: msteinmetz@aip.de
the RAVE collaboration
Affiliation:
Leibniz-Institut für Astrophysik Potsdam (AIP), An der Sternwarte 16, 14482 Potsdam, Germany, email: msteinmetz@aip.de
Rights & Permissions [Opens in a new window]

Abstract

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The 5th RAVE data release is based on 520,781 spectra (R ≈ 7500 in the CaT region at 8410 - 8795Å) of 457,588 unique stars. RAVE DR5 provides radial velocities, stellar parameters and individual abundances for up to seven elements and distances found using isochrones for a considerable subset of these objects. In particular, RAVE DR5 has 255,922 stellar observations that also have parallaxes and proper motions from the Tycho-Gaia astrometric solution (TGAS) in Gaia DR1. The combination of RAVE and TGAS thus provides the currently largest overlap of spectroscopic and space-based astrometric data and thus can serve as a formidable preview of what Gaia is going to deliver in coming data releases. Basic properties of the RAVE+TGAS survey and its derived data products are presented as well as first applications w.r.t wave-like patterns in the disk structure. An outlook to the 6th RAVE data release is given.

Keywords

Galaxy: abundances, disk, kinematics and dynamics, structureastronomical data bases: surveys
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 13 , Symposium S334: Rediscovering our Galaxy , July 2017 , pp. 116 - 119
Copyright
Copyright © International Astronomical Union 2018 

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