The milky way tomography with SDSS. I. Stellar number density distribution

Astrophysical Journal

Volumn 673, Issue 2, 2008, Pages 864-914

  Jurić, Mario ^a,b   Ivezić, Željko ^c   Brooks, Alyson ^c   Lupton, Robert H ^a   Schlegel, David ^a,d   Finkbeiner, Douglas ^a,e   Padmanabhan, Nikhil ^a,d   Bond, Nicholas ^a   Sesar, Branimir ^c   Rockosi, Constance M ^c,f   Knapp, Gillian R ^a   Gunn, James E ^a   Sumi, Takahiro ^a,g   Schneider, Donald P ^h   Barentine, J C ⁱ   Brewington, Howard J ⁱ   Brinkmann, J ⁱ   Fukugita, Masataka ^j   Harvanek, Michael ⁱ   Kleinman, S J ⁱ   Krzesinski, Jurek ^i,k   Long, Dan ⁱ   Neilsen Jr , Eric H ^l   Nitta, Atsuko ⁱ   Snedden, Stephanie A ⁱ   York, Donald G ^m   more..

^a PRINCETON UNIVERSITY   (United States)

^b INSTITUTE FOR ADVANCED STUDY   (United States)

^c UNIVERSITY OF WASHINGTON   (United States)

^d LAWRENCE BERKELEY NATIONAL LABORATORY   (United States)

^e HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^f UNIVERSITY OF CALIFORNIA   (United States)

^g NAGOYA UNIVERSITY   (Japan)

^h PENNSYLVANIA STATE UNIVERSITY   (United States)

ⁱ APACHE POINT OBSERVATORY   (United States)

^j UNIVERSITY OF TOKYO   (Japan)

^k PEDAGOGICAL UNIVERSITY   (Poland)

^l FERMI NATIONAL ACCELERATOR LABORATORY   (United States)

^m UNIVERSITY OF CHICAGO   (United States)

more..

Author keywords

Galaxy: disk; Galaxy: fundamental parameters; Galaxy: halo; Galaxy: structure

Indexed keywords

EID: 40249099163     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/523619     Document Type: Article

References (137)