Hubble space telescope imaging of Lyα emission at z ≈ 4.4

Astrophysical Journal

Volumn 735, Issue 1, 2011, Pages

  Finkelstein, Steven L ^a   Cohen, Seth H ^b   Windhorst, Rogier A ^b   Ryan, Russell E ^c   Hathi, Nimish P ^d   Finkelstein, Keely D ^a   Anderson, Jay ^e   Grogin, Norman A ^e   Koekemoer, Anton M ^e   Malhotra, Sangeeta ^b   Mutchler, Max ^e   Rhoads, James E ^b   McCarthy, Patrick J ^d   O'Connell, Robert W ^f   Balick, Bruce ^g   Bond, Howard E ^e   Calzetti, Daniela ^h   Disney, Michael J ⁱ   Dopita, Michael A ^j   Frogel, Jay A ^k   Hall, Donald N B ^l   Holtzman, Jon A ^m   Kimble, Randy A ⁿ   Luppino, Gerard ^l   Paresce, Francesco ^o   Saha, Abhijit ^p   Silk, Joseph I ^q   Trauger, John T ^r   Walker, Alistair R ^s   Whitmore, Bradley C ^e   Young, Erick T ^t   more..

^a TEXAS A AND M UNIVERSITY   (United States)

^b ARIZONA STATE UNIVERSITY   (United States)

^c UNIVERSITY OF CALIFORNIA   (United States)

^d CARNEGIE OBSERVATORIES   (United States)

^e NASA Hubble Fellowship Program   (United States)

^f UNIVERSITY OF VIRGINIA   (United States)

^g UNIVERSITY OF WASHINGTON   (United States)

^h UNIVERSITY OF MASSACHUSETTS   (United States)

ⁱ CARDIFF UNIVERSITY   (United Kingdom)

^j AUSTRALIAN NATIONAL UNIVERSITY   (Australia)

^k University of Space Research Association   (United States)

^l UNIVERSITY OF HAWAII   (United States)

^m NEW MEXICO STATE UNIVERSITY   (United States)

ⁿ NASA GODDARD SPACE FLIGHT CENTER   (United States)

^o OSSERVATORIO ASTRONOMICO DI BOLOGNA   (Italy)

^p NATIONAL OPTICAL ASTRONOMY OBSERVATORY   (United States)

^q UNIVERSITY OF OXFORD   (United Kingdom)

^r CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^s CERRO TOLOLO INTER AMERICAN OBSERVATORY   (Chile)

^t NASA AMES RESEARCH CENTER   (United States)

more..

Author keywords

galaxies: evolution; galaxies: high redshift; galaxies: ISM

Indexed keywords

EID: 79960009744     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1088/0004-637X/735/1/5     Document Type: Article

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