The udf05 follow-up of the hubble ultra deep field. III. the luminosity function at z ∼ 6

Astrophysical Journal

Volumn 738, Issue 2, 2011, Pages

  Su, Jian ^a,b   Stiavelli, Massimo ^b   Oesch, Pascal ^c,d   Trenti, Michele ^e   Bergeron, Eddie ^b   Bradley, Larry ^b   Carollo, Marcella ^c   Dahlen, Tomas ^b   Ferguson, Henry C ^b   Giavalisco, Mauro ^f   Koekemoer, Anton ^b   Lilly, Simon ^c   Lucas, Ray A ^b   Mobasher, Bahram ^g   Panagia, Nino ^b,h,i   Pavlovsky, Cheryl ^b  

^a JOHNS HOPKINS UNIVERSITY   (United States)

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

^c ETH ZURICH   (Switzerland)

^d University of California at Santa Cruz   (United States)

^e UNIVERSITY OF COLORADO   (United States)

^f UNIVERSITY OF MASSACHUSETTS   (United States)

^g UNIVERSITY OF CALIFORNIA   (United States)

^h INAF OSSERVATORIO ASTROFISICO DI CATANIA   (Italy)

ⁱ SUPERNOVA LTD   (Virgin Islands (British))

Author keywords

galaxies: evolution; galaxies: formation; galaxies: high redshift; galaxies: luminosity function, mass function; methods: data analysis

Indexed keywords

EID: 80052808101     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1088/0004-637X/738/2/123     Document Type: Article

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