The Astrophysical Journal, 684:287–325, 2008 September 1 A # 2008. The American Astronomical Society. All rights reserved. Printed in U.S.A.
THE MILKY WAY TOMOGRAPHY WITH SDSS. II. STELLAR METALLICITY Zˇ eljko Ivezic´,1 Branimir Sesar,1 Mario Juric´,2 Nicholas Bond,3 Julianne Dalcanton,1 Constance M. Rockosi,4 Brian Yanny,5 Heidi J. Newberg,6 Timothy C. Beers,7 Carlos Allende Prieto,8 Ron Wilhelm,9 Young Sun Lee,7 Thirupathi Sivarani,7 John E. Norris,10 Coryn A. L. Bailer-Jones,11 Paola Re Fiorentin,11,12 David Schlegel,13 Alan Uomoto,14 Robert H. Lupton,3 Gillian R. Knapp,3 James E. Gunn,3 Kevin R. Covey,15 J. Allyn Smith,16 Gajus Miknaitis,5 Mamoru Doi,17 Masayuki Tanaka,18 Masataka Fukugita,19 Steve Kent,5 Douglas Finkbeiner,15 Jeffrey A. Munn,20 Jeffrey R. Pier,20 Tom Quinn,1 Suzanne Hawley,1 Scott Anderson,1 Furea Kiuchi,1 Alex Chen,1 James Bushong,1 Harkirat Sohi,1 Daryl Haggard,1 Amy Kimball,1 John Barentine,21 Howard Brewington,21 Mike Harvanek,21 Scott Kleinman,21 Jurek Krzesinski,21 Dan Long,21 Atsuko Nitta,21 Stephanie Snedden,21 Brian Lee,13 Hugh Harris,20 Jonathan Brinkmann,21 Donald P. Schneider,22 and Donald G. York23 Received 2007 October 4; accepted 2008 April 22
ABSTRACT Using effective temperature and metallicity derived from SDSS spectra for 60,000 F- and G-type main-sequence stars (0:2