The UDF05 follow-up of the hubble ultra deep field. I. The faint-end slope of the Lyman break galaxy population at z ∼ 51

Astrophysical Journal

Volumn 671, Issue 2, 2007, Pages 1212-1216

  Oesch, P A ^a   Stiavelli, M ^b,c   Carollo, C M ^a   Bergeron, L E ^b   Koekemoer, A M ^b   Lucas, R A ^b   Pavlovsky, C M ^b   Trenti, M ^b   Lilly, S J ^a   Beckwith, S V W ^b   Dahlen, T ^b   Ferguson, H C ^b   Gardner, Jonathan P ^d   Lacey, C ^e   Mobasher, B ^b   Panagia, N ^b,f,g   Rix, H W ^h  

^a ETH ZURICH   (Switzerland)

^b STScI   (United States)

^c JOHNS HOPKINS UNIVERSITY   (United States)

^d NASA GODDARD SPACE FLIGHT CENTER   (United States)

^e DURHAM UNIVERSITY   (United Kingdom)

^f INAF OSSERVATORIO ASTROFISICO DI CATANIA   (Italy)

^g SUPERNOVA LTD   (Virgin Islands (British))

^h MAX PLANCK INSTITUT FÜR ASTRONOMIE   (Germany)

Author keywords

Dark matter; Galaxies: evolution; Galaxies: formation; Galaxies: high redshift; Galaxies: luminosity function, mass function

Indexed keywords

EID: 40249116693     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/522423     Document Type: Article

References (59)