THE SEGUE STELLAR PARAMETER PIPELINE. III. COMPARISON WITH HIGH-RESOLUTION SPECTROSCOPY OF SDSS/SEGUE FIELD STARS
Top Cited Papers
- 13 October 2008
- journal article
- Published by American Astronomical Society in The Astronomical Journal
- Vol. 136 (5) , 2070-2082
- https://doi.org/10.1088/0004-6256/136/5/2070
Abstract
No abstract availableAll Related Versions
This publication has 53 references indexed in Scilit:
- Elemental abundance survey of the Galactic thick discMonthly Notices of the Royal Astronomical Society, 2006
- Analysis of the carbon-rich very metal-poor dwarf G77–61Astronomy & Astrophysics, 2005
- The Geneva-Copenhagen survey of the Solar neighbourhoodAstronomy & Astrophysics, 2004
- On the Galactic chemical evolution of sulfurAstronomy & Astrophysics, 2004
- Kinetic equilibrium of iron in the atmospheres of cool starsAstronomy & Astrophysics, 2003
- Sulphur abundances in disk stars: A correlation with siliconAstronomy & Astrophysics, 2002
- A Survey of Proper-Motion Stars. XIV. Spectroscopic Binaries among Metal-poor Field Blue StragglersThe Astronomical Journal, 2001
- A database of high and medium-resolution stellar spectraAstronomy & Astrophysics, 2001
- The Sloan Digital Sky Survey: Technical SummaryThe Astronomical Journal, 2000
- The Sloan Digital Sky Survey Photometric SystemThe Astronomical Journal, 1996