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

Abstract:

Gravitational lensing is a powerful astrophysical and cosmological probe and is particularly valuable at submillimeter wavelengths for the study of the statistical and individual properties of dusty star-forming galaxies. However, the identification of gravitational lenses is often time-intensive, involving the sifting of large volumes of imaging or spectroscopic data to find few candidates. We used early data from the Herschel Astrophysical Terahertz Large Area Survey to demonstrate that wid...

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Publication status:
Published

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Publisher copy:
10.1126/science.1193420

Authors


Negrello, M More by this author
Hopwood, R More by this author
De Zotti, G More by this author
More by this author
Institution:
University of Oxford
Department:
Oxford, MPLS, Physics, Astrophysics
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Journal:
Science (New York, N.Y.)
Volume:
330
Issue:
6005
Pages:
800-804
Publication date:
2010-11-05
DOI:
EISSN:
1095-9203
ISSN:
0036-8075
URN:
uuid:41c4557e-e0a8-409f-bd18-101f7386cfa1
Source identifiers:
93196
Local pid:
pubs:93196
Language:
English
Keywords:

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