Unveiling the nature of submillimeter galaxy SXDF 850.6

Astrophysical Journal

Volumn 711, Issue 2, 2010, Pages 974-979

  Hatsukade, B ^a   Iono, D ^b   Akiyama, T ^c   Yoshikawa, M ^c   Dunlop, J S ^d   Ivison, R J ^d,e   Peck, A B ^f   Ikarashi, S ^a   Biggs, A ^g   Ezawa, H ^b   Hanami, H ^h   Ho, P ⁱ   Hughes, D H ^j   Kawabe, R ^b   Kohno, K ^a,k   Matsushita, S ⁱ   Nakanishi, K ^b   Padilla, N ^l   Petitpas, G ^m   Tamura, Y ^b   Wagg, J ^j,m,n   Wilner, D J ^m   Wilson, G W ^o   Yamada, T ^c   Yun, M S ^o   more..

^a UNIVERSITY OF TOKYO   (Japan)

^b NATIONAL ASTRONOMICAL OBSERVATORY OF JAPAN   (Japan)

^c TOHOKU UNIVERSITY   (Japan)

^d UNIVERSITY OF EDINBURGH   (United Kingdom)

^e UK ASTRONOMY TECHNOLOGY CENTRE   (United Kingdom)

^f JOINT ALMA OBSERVATORY   (Chile)

^g EUROPEAN SOUTHERN OBSERVATORY   (Germany)

^h IWATE UNIVERSITY   (Japan)

ⁱ INSTITUTE OF ASTRONOMY AND ASTROPHYSICS   (Taiwan)

^j INSTITUTO NACIONAL DE ASTROFÍSICA   (Mexico)

^k UNIVERSITY OF TOKYO   (Japan)

^l PONTIFICIA UNIVERSIDAD CATÓLICA DE CHILE   (Chile)

^m HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

ⁿ EUROPEAN SOUTHERN OBSERVATORY   (Chile)

^o UNIVERSITY OF MASSACHUSETTS   (United States)

more..

Author keywords

Cosmology: observations; Galaxies: evolution; Galaxies: formation; Galaxies: high redshift; Galaxies: starburst; Submillimeter: galaxies

Indexed keywords

EID: 77649227340     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1088/0004-637X/711/2/974     Document Type: Article

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