The stellar content of the COSMOS field as derived from morphological and sed-based star/galaxy separation

Astrophysical Journal, Supplement Series

Volumn 172, Issue 1, 2007, Pages 545-559

  Robin, A C ^a   Rich, R M ^b   Aussel, H ^c,d   Capak, P ^e   Tasca, L A M ^f   Jahnke, K ^g   Kakazu, Y ^c   Kneib, J P ^f   Koekemoer, A ^h   Leauthaud, A C ^f   Lilly, S ⁱ   Mobasher, B ^h   Scoville, N ^e,j   Taniguchi, Y ^k   Thompson, D J ^e,l  

^a UNIVERSITÉ DE FRANCHE COMTÉ   (France)

^b UNIVERSITY OF CALIFORNIA   (United States)

^c UNIVERSITY OF HAWAII   (United States)

^d UNIVERSITÉ PARIS DIDEROT   (France)

^e CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^f AIX MARSEILLE UNIVERSITÉ   (France)

^g MAX PLANCK INSTITUT FÜR ASTRONOMIE   (Germany)

^h STScI   (United States)

ⁱ ETH ZURICH   (Switzerland)

^j UNIVERSITY OF HAWAII   (United States)

^k EHIME UNIVERSITY   (Japan)

^l UNIVERSITY OF ARIZONA   (United States)

more..

Author keywords

Galaxy: halo; Galaxy: stellar content; Galaxy: structure; Stars: low mass, brown dwarfs; Stars: statistics; White dwarfs

Indexed keywords

EID: 35348851270     PISSN: 00670049     EISSN: None     Source Type: Journal    
DOI: 10.1086/516600     Document Type: Article

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