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The Milky Way Tomography with SDSS: II. Stellar Metallicity (2008) |
- Ivezic, Zeljko,
- Sesar, Branimir,
- Juric, Mario,
- Bond, Nicholas,
- Dalcanton, Julianne,
- Rockosi, Constance M.,
- Yanny, Brian,
- Newberg, Heidi J.,
- Beers, Timothy C.,
- Prieto, Carlos Allende,
- Wilhelm, Ron,
- Lee, Young Sun,
- Sivarani, Thirupathi,
- Norris, John E.,
- Fiorentin, Paola Re,
- Schlegel, David,
- Uomoto, Alan,
- Lupton, Robert H.,
- Knapp, Gillian R.,
- Gunn, James E.,
- Covey, Kevin R.,
- Smith, J. Allyn,
- Miknaitis, Gajus,
- Doi, Mamoru,
- Tanaka, Masayuki,
- Fukugita, Masataka,
- Kent, Steve,
- Finkbeiner, Douglas,
- Munn, Jeffrey A.,
- Pier, Jeffrey R.,
- Quinn, Tom,
- Hawley, Suzanne,
- Anderson, Scott,
- Kiuchi, Furea,
- Chen, Alex,
- Bushong, James,
- Sohi, Harkirat,
- Haggard, Daryl,
- Kimball, Amy,
- Barentine, John,
- Brewington, Howard,
- Harvanek, Mike,
- Kleinman, Scott,
- Krzesinski, Jurek,
- Long, Dan,
- Nitta, Atsuko,
- Snedden, Stephanie,
- Lee, Brian,
- Harris, Hugh,
- Brinkmann, Jonathan,
- Schneider, Donald P.,
- York, Donald G.
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Abstract |
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Using effective temperature and metallicity derived from SDSS spectra for ~60,000 F and G type main sequence stars (0.2.
Comment: 40 pages, 21 figures, emulateApJ style, accepted to ApJ, high resolution figures are available from http://www.astro.washington.edu/ivezic/sdss/mw/astroph0804.3850 |
Publication details |
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