An overdensity of galaxies at z = 5.9 ± 0.2 in the hubble ultra deep field confirmed using the ACS grism

Astrophysical Journal

Volumn 626, Issue 2 I, 2005, Pages 666-679

  Malhotra, S ^a   Rhoads, J E ^a   Pirzkal, N ^a   Haiman, Z ^b   Xu, C ^a   Daddi, E ^c,d   Yan, H ^e   Bergeron, L E ^a   Wang, J ^a,f   Ferguson, H C ^a   Gronwall, C ^g   Koekemoer, A ^a   Kuemmel, M ^d   Moustakas, L A ^a   Panagia, N ^a,h   Pasquali, A ⁱ   Stiavelli, M ^a   Walsh, J ^d   Windhorst, R A ^j   Di Serego Alighieri, S ^k  

^a STScI   (United States)

^b Och Spine at New York Presbyterian Hospitals   (United States)

^c EUROPEAN SOUTHERN OBSERVATORY   (Germany)

^d NATIONAL OPTICAL ASTRONOMY OBSERVATORY   (United States)

^e CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^f UNIVERSITY OF SCIENCE AND TECHNOLOGY OF CHINA   (China)

^g PENNSYLVANIA STATE UNIVERSITY   (United States)

^h ESA

ⁱ ETH ZURICH   (Switzerland)

^j ARIZONA STATE UNIVERSITY   (United States)

^k INAF OSSERVATORIO ASTROFISICO DI ARCETRI   (Italy)

more..

Author keywords

Galaxies: evolution; Galaxies: formation; Galaxies: high redshift; Galaxies: luminosity function, mass function; Intergalactic medium

Indexed keywords

EID: 23844548908     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/430047     Document Type: Article

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