The detection of a population of submillimeter-bright, strongly lensed galaxies

Science

Volumn 330, Issue 6005, 2010, Pages 800-804

  Negrello, Mattia ^a   Hopwood, R ^a   De Zotti, G ^b,c   Cooray, A ^d   Verma, A ^e   Bock, J ^f,g   Frayer, D T ^h   Gurwell, M A ⁱ   Omont, A ^j   Neri, R ^k   Dannerbauer, H ^l   Leeuw, L L ^m,n   Barton, E ^d   Cooke, J ^d,g   Kim, S ^d   Da Cunha, E ^o   Rodighiero, G ^p   Cox, P ^k   Bonfield, D G ^q   Jarvis, M J ^q   Serjeant, S ^a   Ivison, R J ^r,s   Dye, S ^t   Aretxaga, I ^u   Hughes, D H ^u   Ibar, E ^r   Bertoldi, F ^v   Valtchanov, I ^w   Eales, S ^t   Dunne, L ^x   Driver, S P ^y   Auld, R ^t   Buttiglione, S ^b   Cava, A ^z,aa   Grady, C A ^ab,ac   Clements, D L ^ad   Dariush, A ^t   Fritz, J ^ae   Hill, D ^y   Hornbeck, J B ^af   Kelvin, L ^y   Lagache, G ^ag,ah   Lopez Caniego, M ^ai   Gonzalez Nuevo, J ^c   Maddox, S ^x   Pascale, E ^t   Pohlen, M ^t   Rigby, E E ^x   Robotham, A ^y   Simpson, C ^aj   Smith, D J B ^x   Temi, P ^ak   Thompson, M A ^q   Woodgate, B E ^ac   York, D G ^al   Aguirre, J E ^am   Beelen, A ^ah   Blain, A ^g   Baker, A J ^an   Birkinshaw, M ^ao   Blundell, R ⁱ   Bradford, C M ^f,g   Burgarella, D ^ap   Danese, L ^c   Dunlop, J S ^r   Fleuren, S ^aq   Glenn, J ^ar   Harris, A I ^as   Kamenetzky, J ^ar   Lupu, R E ^am   Maddalena, R J ^h   Madore, B F ^at   Maloney, P R ^ar   Matsuhara, H ^au   Michaowski, M J ^s   Murphy, E J ^av   Naylor, B J ^f   Nguyen, H ^f   Popescu, C ^aw   Rawlings, S ^e   Rigopoulou, D ^e,ax   Scott, D ^ay   Scott, K S ^am   Seibert, M ^at   Smail, I ^az   Tuffs, R J ^ba   Vieira, J D ^g   Van Der Werf, P P ^s,bb   Zmuidzinas, J ^f,g   more..

^a OPEN UNIVERSITY   (United Kingdom)

^b INAF OSSERVATORIO ASTRONOMICO DI PADOVA   (Italy)

^c SISSA   (Italy)

^d UNIVERSITY OF CALIFORNIA   (United States)

^e UNIVERSITY OF OXFORD   (United Kingdom)

^f CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^g CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^h NATIONAL RADIO ASTRONOMY OBSERVATORY   (United States)

ⁱ HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^j INSTITUT D'ASTROPHYSIQUE DE PARIS   (France)

^k IRAM   (France)

^l UNIVERSITÉ PARIS DIDEROT   (France)

^m UNIVERSITY OF JOHANNESBURG   (South Africa)

ⁿ SETI INSTITUTE   (United States)

^o UNIVERSITY OF CRETE   (Greece)

^p UNIVERSITY OF PADOVA   (Italy)

^q UNIVERSITY OF HERTFORDSHIRE   (United Kingdom)

^r UK ASTRONOMY TECHNOLOGY CENTRE   (United Kingdom)

^s UNIVERSITY OF EDINBURGH   (United Kingdom)

^t CARDIFF UNIVERSITY   (United Kingdom)

^u INSTITUTO NACIONAL DE ASTROFÍSICA   (Mexico)

^v UNIVERSITY OF BONN   (Germany)

^w EUROPEAN SPACE AGENCY   (Spain)

^x UNIVERSITY OF NOTTINGHAM   (United Kingdom)

^y UNIVERSITY OF ST ANDREWS   (United Kingdom)

^z INSTITUTO DE ASTROFÍSICA DE CANARIAS   (Spain)

^aa UNIVERSIDAD DE LA LAGUNA   (Spain)

^ab EUREKA SCIENTIFIC   (United States)

^ac NASA GODDARD SPACE FLIGHT CENTER   (United States)

^ad IMPERIAL COLLEGE LONDON   (United Kingdom)

^ae GHENT UNIVERSITY   (Belgium)

^af UNIVERSITY OF LOUISVILLE   (United States)

^ag UNIVERSITÉ PARIS SUD   (France)

^ah UNIVERSITÉ PARIS SACLAY   (France)

^ai INSTITUTO DE FÍSICA DE CANTABRIA CSIC UC   (Spain)

^aj LIVERPOOL JOHN MOORES UNIVERSITY   (United Kingdom)

^ak NASA AMES RESEARCH CENTER   (United States)

^al UNIVERSITY OF CHICAGO   (United States)

^am UNIVERSITY OF PENNSYLVANIA   (United States)

^an RUTGERS UNIVERSITY   (United States)

^ao UNIVERSITY OF BRISTOL   (United Kingdom)

^ap AIX MARSEILLE UNIVERSITÉ   (France)

^aq QUEEN MARY UNIVERSITY OF LONDON   (United Kingdom)

^ar UNIVERSITY OF COLORADO   (United States)

^as Bldg 142   (United States)

^at CARNEGIE OBSERVATORIES   (United States)

^au JAPAN AEROSPACE EXPLORATION AGENCY   (Japan)

^av CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^aw UNIVERSITY OF CENTRAL LANCASHIRE   (United Kingdom)

^ax RUTHERFORD APPLETON LABORATORY   (United Kingdom)

^ay UNIVERSITY OF BRITISH COLUMBIA   (Canada)

^az DURHAM UNIVERSITY   (United Kingdom)

^ba MAX PLANCK INSTITUT FÜR KERNPHYSIK   (Germany)

^bb LEIDEN UNIVERSITY   (Netherlands)

more..

Author keywords

[No Author keywords available]

Indexed keywords

ASTROPHYSICS; COSMOLOGY; DATA SET; DETECTION METHOD; SPECTROSCOPY; SURVEY; VOLUME; WAVELENGTH;

ARTICLE; ASTRONOMY; GRAVITY; IMAGING; OPTICAL INSTRUMENTATION; PRIORITY JOURNAL; PRODUCTIVITY; SPECTROSCOPY; SUBMILLIMETER GALAXY;

EID: 78149295965     PISSN: 00368075     EISSN: 10959203     Source Type: Journal    
DOI: 10.1126/science.1193420     Document Type: Article

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55. Herschel is an ESA space observatory with science instruments provided by European-led principal investigator consortia and with important participation from NASA. U.S. participants in H-ATLAS acknowledge support from NASA through a contract from JPL. This work was supported by the Science and Technology Facilities Council (grants PP/D002400/1 and ST/G002533/1) and studentship SF/F005288/1. We thank Agenzia Spaziale Italiana (ASI) for funding through contract No. I/016/07/0 COFIS and ASI/Istituto Nazionale di Astrofisica agreement I/072/09/0 for the Planck Low-Frequency Instrument (LFI) Activity of Phase E2. Research supported in part by Consejo Nacional de Ciencia y Tecnología (CONACyT) grants 39953-F and 39548-F. The W. M. Keck Observatory is operated as a scientific partnership among the California Institute of Technology, the University of California, and NASA. The Observatory was made possible by the generous financial support of the W. M. Keck Foundation. The Submillimeter Array is a joint project between the Smithsonian Astrophysical Observatory and the Academia Sinica Institute of Astronomy and Astrophysics and is funded by the Smithsonian Institution and the Academia Sinica. IRAM is supported by Institut National des Sciences de l'Univers (INSU)/CNRS (France), Max Planck Society (MPG) (Germany), and Instituto Geográfico Nacional (IGN) (Spain). Z-spec was supported by NSF grant AST-0807990 to J.A. and by the CSO NSF Cooperative Agreement AST-0838261. Support was provided to J.K. by an NSF Graduate Research Fellowship. Z-spec was constructed under NASA SARA grants NAGS-11911 and NAGS-12788 and an NSF Career grant (AST-0239270) and a Research Corporation Award (RI0928) to J.G., in collaboration with JPL, California Institute of Technology, under a contract with NASA. Construction of and observations with the Zpectrometer have been supported by NSF grants AST-0503946 and AST-0708653. NRAO is a facility of the NSF operated under cooperative agreement by Associated Universities. The optical spectroscopic redshift of ID130 was derived from observations obtained with the Apache Point Observatory 3.5-m telescope, which is owned and operated by the Astrophysical Research Consortium. The optical spectroscopic redshifts of ID9 and ID11 were obtained with the William Herschel Telescope, which is operated on the island of La Palma by the Isaac Newton Group in the Spanish Observatorio del Roque de los Muchachos of the Instituto de Astrofísica de Canarias. For the use of Keck, SMA, and CSO, the authors wish to recognize and acknowledge the very important cultural role and reverence that the summit of Mauna Kea has always had within the indigenous Hawaiian community. We are most fortunate to have the opportunity to conduct observations from this mountain.