Galaxy stellar mass assembly between 0.2 < z < 2 from the s-cosmos survey

Astrophysical Journal

Volumn 709, Issue 2, 2010, Pages 644-663

  Ilbert, O ^a,b   Salvato, M ^c   Le Floc'H, E ^a   Aussel, H ^d   Capak, P ^c,e   McCracken, H J ^f   Mobasher, B ^g   Kartaltepe, J ^a   Scoville, N ^c   Sanders, D B ^a   Arnouts, S ^h   Bundy, K ⁱ   Cassata, P ^b   Kneib, J P ^b   Koekemoer, A ^j   Le Fevre O ^b   Lilly, S ^k   Surace, J ^e   Taniguchi, Y ^l   Tasca, L ⁱ   Thompson, D ^c,m   Tresse, L ^b   Zamojski, M ^c   Zamorani, G ⁿ   Zucca, E ⁿ   more..

^a UNIVERSITY OF HAWAII   (United States)

^b AIX MARSEILLE UNIVERSITÉ   (France)

^c CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^d UNIVERSITÉ PARIS DIDEROT   (France)

^e CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^f INSTITUT D'ASTROPHYSIQUE DE PARIS   (France)

^g UNIVERSITY OF CALIFORNIA   (United States)

^h CANADA FRANCE HAWAII TELESCOPE   (United States)

ⁱ UNIVERSITY OF TORONTO   (Canada)

^j AURA for the European Space Agency   (United States)

^k ETH ZURICH   (Switzerland)

^l EHIME UNIVERSITY   (Japan)

^m UNIVERSITY OF ARIZONA   (United States)

ⁿ INAF OSSERVATORIO ASTRONOMICO DI BOLOGNA   (Italy)

more..

Author keywords

Galaxies: evolution; Galaxies: formation; Galaxies: luminosity function, mass function

Indexed keywords

EID: 73949135782     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1088/0004-637X/709/2/644     Document Type: Article

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