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The Milky Way Tomography with SDSS. II. Stellar Metallicity

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dc.contributor.authorIvezic, Zeljko
dc.contributor.authorSesar, Branimir
dc.contributor.authorJuric, Mario
dc.contributor.authorBond, Nicholas
dc.contributor.authorDalcanton, Julianne
dc.contributor.authorRockosi, Constance
dc.contributor.authorYanny, Brian
dc.contributor.authorNewberg, Heidi Jo
dc.contributor.authorBeers, Timothy C
dc.contributor.authorAllende Prieto, C
dc.contributor.authorWilhelm, Ronald
dc.contributor.authorNorris, John
dc.date.accessioned2015-12-08T22:26:53Z
dc.date.issued2008
dc.date.updated2015-12-08T09:15:17Z
dc.description.abstractUsing effective temperature and metallicity derived from SDSS spectra for ∼60,000 F- and G-type main-sequence stars (0.2 < g - r < 0.6), we develop polynomial models for estimating these parameters from the SDSS u - g and g - r colors. These photometric
dc.identifier.issn0004-637X
dc.identifier.urihttp://hdl.handle.net/1885/33826
dc.publisherIOP Publishing
dc.sourceAstrophysical Journal, The
dc.subjectKeywords: Galaxy: Halo; Galaxy: Kinematics and dynamics; Galaxy: Stellar content; Galaxy: Structure; Methods: Data analysis; Stars: Statistics
dc.titleThe Milky Way Tomography with SDSS. II. Stellar Metallicity
dc.typeJournal article
local.bibliographicCitation.lastpage325
local.bibliographicCitation.startpage287
local.contributor.affiliationIvezic, Zeljko, University of Washington
local.contributor.affiliationSesar, Branimir, University of Washington
local.contributor.affiliationJuric, Mario, Princeton University
local.contributor.affiliationBond, Nicholas, Princeton University
local.contributor.affiliationDalcanton, Julianne, University of Washington
local.contributor.affiliationRockosi, Constance, University of California
local.contributor.affiliationYanny, Brian, Fermi National Accelerator Laboratory
local.contributor.affiliationNewberg, Heidi Jo, Rensselaer Polytechnic Institute
local.contributor.affiliationBeers, Timothy C, Michigan State University
local.contributor.affiliationAllende Prieto, C, University of Texas
local.contributor.affiliationWilhelm, Ronald, Texas Tech University
local.contributor.affiliationNorris, John, College of Physical and Mathematical Sciences, ANU
local.contributor.authoruidNorris, John, u7401084
local.description.embargo2037-12-31
local.description.notesImported from ARIES
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.ariespublicationu4362859xPUB106
local.identifier.citationvolume684
local.identifier.doi10.1086/589678
local.identifier.scopusID2-s2.0-52049086910
local.identifier.thomsonID000258730700022
local.type.statusPublished Version

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