4.6 Article

THE SLOAN DIGITAL SKY SURVEY DATA RELEASE 7 SPECTROSCOPIC M DWARF CATALOG. I. DATA

Journal

ASTRONOMICAL JOURNAL
Volume 141, Issue 3, Pages -

Publisher

IOP PUBLISHING LTD
DOI: 10.1088/0004-6256/141/3/97

Keywords

brown dwarfs; Galaxy: kinematics and dynamics; stars: abundances; stars: activity; stars: late-type; stars: low-mass

Funding

  1. NSF [06-07644]
  2. NASA [HST-HF-51253.01-A, NAS 5-26555]
  3. Alfred P. Sloan Foundation
  4. National Science Foundation
  5. U.S. Department of Energy
  6. Japanese Monbukagakusho
  7. Max Planck Society
  8. Higher Education Funding Council for England
  9. American Museum of Natural History
  10. Astrophysical Institute Potsdam
  11. University of Basel
  12. University of Cambridge
  13. Case Western Reserve University
  14. University of Chicago
  15. Drexel University
  16. Fermilab
  17. Institute for Advanced Study
  18. Japan Participation Group
  19. Johns Hopkins University
  20. Joint Institute for Nuclear Astrophysics
  21. Kavli Institute for Particle Astrophysics and Cosmology
  22. Korean Scientist Group
  23. Chinese Academy of Sciences (LAMOST)
  24. Los Alamos National Laboratory
  25. Max-Planck-Institute for Astronomy (MPIA)
  26. Max-Planck-Institute for Astrophysics (MPA)
  27. New Mexico State University
  28. Ohio State University
  29. University of Pittsburgh
  30. University of Portsmouth
  31. Princeton University
  32. United States Naval Observatory
  33. University of Washington
  34. Division Of Astronomical Sciences
  35. Direct For Mathematical & Physical Scien [0909463] Funding Source: National Science Foundation

Ask authors/readers for more resources

We present a spectroscopic catalog of 70,841 visually inspected M dwarfs from the seventh data release of the Sloan Digital Sky Survey. For each spectrum, we provide measurements of the spectral type, a number of molecular band heads, and the H alpha, H beta, H gamma, H delta, and Ca II K emission lines. In addition, we calculate the metallicity-sensitive parameter zeta and identify a relationship between zeta and the g - r and r - z colors of M dwarfs. We assess the precision of our spectral types (which were assigned by individual examination), review the bulk attributes of the sample, and examine the magnetic activity properties of M dwarfs, in particular those traced by the higher order Balmer transitions. Our catalog is cross-matched to Two Micron All Sky Survey infrared data, and contains photometric distances for each star. Finally, we identify eight new late-type M dwarfs that are possibly within 25 pc of the Sun. Future studies will use these data to thoroughly examine magnetic activity and kinematics in late-type M dwarfs and examine the chemical and dynamical history of the local Milky Way.

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