4.6 Article

THE RADIAL VELOCITY EXPERIMENT (RAVE): FOURTH DATA RELEASE

Journal

ASTRONOMICAL JOURNAL
Volume 146, Issue 5, Pages -

Publisher

IOP PUBLISHING LTD
DOI: 10.1088/0004-6256/146/5/134

Keywords

catalogs; stars: abundances; stars: fundamental parameters; surveys; techniques: spectroscopic

Funding

  1. Australian Astronomical Observatory
  2. Leibniz-Institut fur Astrophysik Potsdam (AIP)
  3. Australian National University
  4. Australian Research Council
  5. French National Research Agency
  6. German Research Foundation [SPP 1177, SFB 881]
  7. European Research Council [ERC-StG 240271 Galactica]
  8. Istituto Nazionale di Astrofisica at Padova
  9. Johns Hopkins University
  10. National Science Foundation of the USA [AST-0908326]
  11. W. M. Keck Foundation
  12. Macquarie University
  13. Netherlands Research School for Astronomy
  14. Natural Sciences and Engineering Research Council of Canada
  15. Slovenian Research Agency
  16. Swiss National Science Foundation
  17. Science & Technology Facilities Council of the UK
  18. Opticon
  19. Strasbourg Observatory
  20. University of Heidelberg
  21. University of Groningen
  22. University of Sydney
  23. STFC [PP/D001528/1, ST/K000985/1, ST/G002479/1, ST/K00106X/1, ST/J00149X/1, PP/D001242/1, ST/G002509/1] Funding Source: UKRI
  24. Science and Technology Facilities Council [ST/K00106X/1, PP/D001528/1, ST/K000985/1, ST/G002509/1, ST/G002479/1, ST/J00149X/1, ST/H00243X/1, PP/D001242/1] Funding Source: researchfish
  25. UK Space Agency [PP/D006570/1, ST/K00056X/1, ST/I000852/1] Funding Source: researchfish

Ask authors/readers for more resources

We present the stellar atmospheric parameters (effective temperature, surface gravity, overall metallicity), radial velocities, individual abundances, and distances determined for 425,561 stars, which constitute the fourth public data release of the RAdial Velocity Experiment (RAVE). The stellar atmospheric parameters are computed using a new pipeline, based on the algorithms of MATISSE and DEGAS. The spectral degeneracies and the Two Micron All Sky Survey photometric information are now better taken into consideration, improving the parameter determination compared to the previous RAVE data releases. The individual abundances for six elements (magnesium, aluminum, silicon, titanium, iron, and nickel) are also given, based on a special-purpose pipeline that is also improved compared to that available for the RAVE DR3 and Chemical DR1 data releases. Together with photometric information and proper motions, these data can be retrieved from the RAVE collaboration Web site and the Vizier database.

Authors

I am an author on this paper
Click your name to claim this paper and add it to your profile.

Reviews

Primary Rating

4.6
Not enough ratings

Secondary Ratings

Novelty
-
Significance
-
Scientific rigor
-
Rate this paper

Recommended

No Data Available
No Data Available