RAVE second data release Virtual Observatory Resource

Authors
  1. Zwitter T.
  2. Siebert A.
  3. Munari U.
  4. Freeman K.C.
  5. Siviero A.
  6. Watson F.G.,Fulbright J.P.
  7. Wyse R.F.G.
  8. Campbell R.
  9. Seabroke G.M.
  10. Williams M.,Steinmetz M.
  11. Bienayme O.
  12. Gilmore G.
  13. Grebel E.K.
  14. Helmi A.
  15. Navarro J.F.,Anguiano B.
  16. Boeche C.
  17. Burton D.
  18. Cass P.
  19. Dawe J.
  20. Fiegert K.
  21. Hartley M.,Russell K.
  22. Veltz L.
  23. Bailin J.
  24. Binney J.
  25. Bland-Hawthorn J.
  26. Brown A.,Dehnen W.
  27. Evans N.W.
  28. Fiorentin P.R.
  29. Fiorucci M.
  30. Gerhard O.
  31. Gibson B.,Kelz A.
  32. Kujken K.
  33. Matijevic G.
  34. Minchev I.
  35. Parker Q.A.
  36. Penarrubia J.,Quillen A.
  37. Read M.A.
  38. Reid W.
  39. Roeser S.
  40. Ruchti G.
  41. Scholz R.-D.,Smith M.C.
  42. Sordo R.
  43. Tolstoi E.
  44. Tomasella L.
  45. Vidrih S.
  46. de Boer E.W.
  47. Published by
    CDS
Abstract

We present the second data release of the Radial Velocity Experiment (RAVE), an ambitious spectroscopic survey to measure radial velocities and stellar atmosphere parameters (temperature, metallicity, surface gravity, and rotational velocity) of up to one million stars using the 6dF multi-object spectrograph on the 1.2m UK Schmidt Telescope of the Anglo-Australian Observatory (AAO). The RAVE program started in 2003, obtaining medium resolution spectra (median R=7500) in the Ca-triplet region (8410-8795{AA}) for southern hemisphere stars drawn from the Tycho-2 and SuperCOSMOS catalogues, in the magnitude range 9<I<12. Following the first data release, the current release doubles the sample of published radial velocities, now containing 51829 radial velocities for 49327 individual stars observed on 141 nights between 2003 April 11 and 2005 March 31. Comparison with external data sets shows that the new data collected since 2004 April 3 show a standard deviation of 1.3km/s, about twice as good as for the first data release. For the first time, this data release contains values of stellar parameters from 22407 spectra of 21121 individual stars. They were derived by a penalized chi-square method using an extensive grid of synthetic spectra calculated from the latest version of Kurucz stellar atmosphere models. From comparison with external data sets, our conservative estimates of errors of the stellar parameters for a spectrum with an average signal-to-noise ratio (S/N) of ~40 are 400K in temperature, 0.5dex in gravity, and 0.2dex in metallicity. We note however that, for all three stellar parameters, the internal errors estimated from repeat RAVE observations of 855 stars are at least a factor 2 smaller. We demonstrate that the results show no systematic offsets if compared to values derived from photometry or complementary spectroscopic analyses. The data release includes proper motions from Starnet2, Tycho-2, and UCAC2 catalogs and photometric measurements from Tycho-2 USNO-B, DENIS, and 2MASS. The data release can be accessed via the RAVE Web site: http://www.rave-survey.org and through CDS.

Keywords
  1. surveys
  2. radial-velocity
  3. milky-way-galaxy
  4. photometry
Bibliographic source Bibcode
2008AJ....136..421Z
See also HTML
https://cdsarc.cds.unistra.fr/viz-bin/cat/III/257
IVOA Identifier IVOID
ivo://CDS.VizieR/III/257

Access

IVOA Table Access TAP
https://tapvizier.cds.unistra.fr/TAPVizieR/tap
Run SQL-like queries with TAP-enabled clients (e.g., TOPCAT).
IVOA Cone Search SCS
For use with a cone search client (e.g., TOPCAT).
https://vizier.cds.unistra.fr/viz-bin/conesearch/III/257/ravedr2?
https://vizier.iucaa.in/viz-bin/conesearch/III/257/ravedr2?
http://vizieridia.saao.ac.za/viz-bin/conesearch/III/257/ravedr2?

History

2010-02-10T14:03:38Z
Resource record created
2010-02-10T14:03:38Z
Created
2011-06-27T15:14:24Z
Updated

Contact

Name
CDS support team
Postal Address
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
E-Mail
cds-question@unistra.fr