The Detection of a Population of Submillimeter-Bright, Strongly Lensed Galaxies

Mattia Negrello; R. Hopwood; G. De Zotti; A. Cooray; A. Verma; J. Bock; D. T. Frayer; M. A. Gurwell; A. Omont; R. Neri; H. Dannerbauer; L. L. Leeuw; E. Barton; J. Cooke; S. Kim; E. da Cunha; G. Rodighiero; P. Cox; D. G. Bonfield; M. J. Jarvis; S. Serjeant; R. J. Ivison; S. Dye; I. Aretxaga; D. H. Hughes; E. Ibar; F. Bertoldi; I. Valtchanov; S. Eales; L. Dunne; S. P. Driver; R. Auld; S. Buttiglione; A. Cava; C. A. Grady; D. L. Clements; A. Dariush; J. Fritz; D. Hill; J. B. Hornbeck; L. Kelvin; G. Lagache; M. Lopez-Caniego; J. Gonzalez-Nuevo; S. Maddox; E. Pascale; M. Pohlen; E. E. Rigby; A. Robotham; C. Simpson; D. J. B. Smith; P. Temi; M. A. Thompson; B. E. Woodgate; D. G. York; J. E. Aguirre; A. Beelen; A. Blain; A. J. Baker; M. Birkinshaw; R. Blundell; C. M. Bradford; D. Burgarella; L. Danese; James Dunlop; S. Fleuren; J. Glenn; A. I. Harris; J. Kamenetzky; R. E. Lupu; R. J. Maddalena; B. F. Madore; P. R. Maloney; H. Matsuhara; Michal Michalowski; E. J. Murphy; B. J. Naylor; H. Nguyen; C. Popescu; S. Rawlings; D. Rigopoulou; D. Scott; K. S. Scott; M. Seibert; I. Smail; R. J. Tuffs; J. D. Vieira; P. P. van der Werf; J. Zmuidzinas

doi:10.1126/science.1193420

The Detection of a Population of Submillimeter-Bright, Strongly Lensed Galaxies

Mattia Negrello, R. Hopwood, G. De Zotti, A. Cooray, A. Verma, J. Bock, D. T. Frayer, M. A. Gurwell, A. Omont, R. Neri, H. Dannerbauer, L. L. Leeuw, E. Barton, J. Cooke, S. Kim, E. da Cunha, G. Rodighiero, P. Cox, D. G. Bonfield, M. J. JarvisS. Serjeant, R. J. Ivison, S. Dye, I. Aretxaga, D. H. Hughes, E. Ibar, F. Bertoldi, I. Valtchanov, S. Eales, L. Dunne, S. P. Driver, R. Auld, S. Buttiglione, A. Cava, C. A. Grady, D. L. Clements, A. Dariush, J. Fritz, D. Hill, J. B. Hornbeck, L. Kelvin, G. Lagache, M. Lopez-Caniego, J. Gonzalez-Nuevo, S. Maddox, E. Pascale, M. Pohlen, E. E. Rigby, A. Robotham, C. Simpson, D. J. B. Smith, P. Temi, M. A. Thompson, B. E. Woodgate, D. G. York, J. E. Aguirre, A. Beelen, A. Blain, A. J. Baker, M. Birkinshaw, R. Blundell, C. M. Bradford, D. Burgarella, L. Danese, James Dunlop, S. Fleuren, J. Glenn, A. I. Harris, J. Kamenetzky, R. E. Lupu, R. J. Maddalena, B. F. Madore, P. R. Maloney, H. Matsuhara, Michal Michalowski, E. J. Murphy, B. J. Naylor, H. Nguyen, C. Popescu, S. Rawlings, D. Rigopoulou, D. Scott, K. S. Scott, M. Seibert, I. Smail, R. J. Tuffs, J. D. Vieira, P. P. van der Werf, J. Zmuidzinas

School of Physics and Astronomy

Research output: Contribution to journal › Article › peer-review

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 wide-area submillimeter surveys can simply and easily detect strong gravitational lensing events, with close to 100% efficiency.

Original language	English
Pages (from-to)	800
Journal	Science
Volume	330
DOIs	https://doi.org/10.1126/science.1193420
Publication status	Published - 1 Nov 2010

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10.1126/science.1193420

http://adsabs.harvard.edu/abs/2010Sci...330..800N

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Negrello, M., Hopwood, R., De Zotti, G., Cooray, A., Verma, A., Bock, J., Frayer, D. T., Gurwell, M. A., Omont, A., Neri, R., Dannerbauer, H., Leeuw, L. L., Barton, E., Cooke, J., Kim, S., da Cunha, E., Rodighiero, G., Cox, P., Bonfield, D. G., ... Zmuidzinas, J. (2010). The Detection of a Population of Submillimeter-Bright, Strongly Lensed Galaxies. Science, 330, 800. https://doi.org/10.1126/science.1193420

@article{dc8ed2e395834b56a5f3250717aec8fd,

title = "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 wide-area submillimeter surveys can simply and easily detect strong gravitational lensing events, with close to 100% efficiency.",

author = "Mattia Negrello and R. Hopwood and {De Zotti}, G. and A. Cooray and A. Verma and J. Bock and Frayer, {D. T.} and Gurwell, {M. A.} and A. Omont and R. Neri and H. Dannerbauer and Leeuw, {L. L.} and E. Barton and J. Cooke and S. Kim and {da Cunha}, E. and G. Rodighiero and P. Cox and Bonfield, {D. G.} and Jarvis, {M. J.} and S. Serjeant and Ivison, {R. J.} and S. Dye and I. Aretxaga and Hughes, {D. H.} and E. Ibar and F. Bertoldi and I. Valtchanov and S. Eales and L. Dunne and Driver, {S. P.} and R. Auld and S. Buttiglione and A. Cava and Grady, {C. A.} and Clements, {D. L.} and A. Dariush and J. Fritz and D. Hill and Hornbeck, {J. B.} and L. Kelvin and G. Lagache and M. Lopez-Caniego and J. Gonzalez-Nuevo and S. Maddox and E. Pascale and M. Pohlen and Rigby, {E. E.} and A. Robotham and C. Simpson and Smith, {D. J. B.} and P. Temi and Thompson, {M. A.} and Woodgate, {B. E.} and York, {D. G.} and Aguirre, {J. E.} and A. Beelen and A. Blain and Baker, {A. J.} and M. Birkinshaw and R. Blundell and Bradford, {C. M.} and D. Burgarella and L. Danese and James Dunlop and S. Fleuren and J. Glenn and Harris, {A. I.} and J. Kamenetzky and Lupu, {R. E.} and Maddalena, {R. J.} and Madore, {B. F.} and Maloney, {P. R.} and H. Matsuhara and Michal Michalowski and Murphy, {E. J.} and Naylor, {B. J.} and H. Nguyen and C. Popescu and S. Rawlings and D. Rigopoulou and D. Scott and Scott, {K. S.} and M. Seibert and I. Smail and Tuffs, {R. J.} and Vieira, {J. D.} and {van der Werf}, {P. P.} and J. Zmuidzinas",

year = "2010",

month = nov,

day = "1",

doi = "10.1126/science.1193420",

language = "English",

volume = "330",

pages = "800",

journal = "Science",

issn = "0036-8075",

publisher = "AMER ASSOC ADVANCEMENT SCIENCE",

}

Negrello, M, Hopwood, R, De Zotti, G, Cooray, A, Verma, A, Bock, J, Frayer, DT, Gurwell, MA, Omont, A, Neri, R, Dannerbauer, H, Leeuw, LL, Barton, E, Cooke, J, Kim, S, da Cunha, E, Rodighiero, G, Cox, P, Bonfield, DG, Jarvis, MJ, Serjeant, S, Ivison, RJ, Dye, S, Aretxaga, I, Hughes, DH, Ibar, E, Bertoldi, F, Valtchanov, I, Eales, S, Dunne, L, Driver, SP, Auld, R, Buttiglione, S, Cava, A, Grady, CA, Clements, DL, Dariush, A, Fritz, J, Hill, D, Hornbeck, JB, Kelvin, L, Lagache, G, Lopez-Caniego, M, Gonzalez-Nuevo, J, Maddox, S, Pascale, E, Pohlen, M, Rigby, EE, Robotham, A, Simpson, C, Smith, DJB, Temi, P, Thompson, MA, Woodgate, BE, York, DG, Aguirre, JE, Beelen, A, Blain, A, Baker, AJ, Birkinshaw, M, Blundell, R, Bradford, CM, Burgarella, D, Danese, L, Dunlop, J, Fleuren, S, Glenn, J, Harris, AI, Kamenetzky, J, Lupu, RE, Maddalena, RJ, Madore, BF, Maloney, PR, Matsuhara, H, Michalowski, M, Murphy, EJ, Naylor, BJ, Nguyen, H, Popescu, C, Rawlings, S, Rigopoulou, D, Scott, D, Scott, KS, Seibert, M, Smail, I, Tuffs, RJ, Vieira, JD, van der Werf, PP & Zmuidzinas, J 2010, 'The Detection of a Population of Submillimeter-Bright, Strongly Lensed Galaxies', Science, vol. 330, pp. 800. https://doi.org/10.1126/science.1193420

TY - JOUR

T1 - The Detection of a Population of Submillimeter-Bright, Strongly Lensed Galaxies

AU - Negrello, Mattia

AU - Hopwood, R.

AU - De Zotti, G.

AU - Cooray, A.

AU - Verma, A.

AU - Bock, J.

AU - Frayer, D. T.

AU - Gurwell, M. A.

AU - Omont, A.

AU - Neri, R.

AU - Dannerbauer, H.

AU - Leeuw, L. L.

AU - Barton, E.

AU - Cooke, J.

AU - Kim, S.

AU - da Cunha, E.

AU - Rodighiero, G.

AU - Cox, P.

AU - Bonfield, D. G.

AU - Jarvis, M. J.

AU - Serjeant, S.

AU - Ivison, R. J.

AU - Dye, S.

AU - Aretxaga, I.

AU - Hughes, D. H.

AU - Ibar, E.

AU - Bertoldi, F.

AU - Valtchanov, I.

AU - Eales, S.

AU - Dunne, L.

AU - Driver, S. P.

AU - Auld, R.

AU - Buttiglione, S.

AU - Cava, A.

AU - Grady, C. A.

AU - Clements, D. L.

AU - Dariush, A.

AU - Fritz, J.

AU - Hill, D.

AU - Hornbeck, J. B.

AU - Kelvin, L.

AU - Lagache, G.

AU - Lopez-Caniego, M.

AU - Gonzalez-Nuevo, J.

AU - Maddox, S.

AU - Pascale, E.

AU - Pohlen, M.

AU - Rigby, E. E.

AU - Robotham, A.

AU - Simpson, C.

AU - Smith, D. J. B.

AU - Temi, P.

AU - Thompson, M. A.

AU - Woodgate, B. E.

AU - York, D. G.

AU - Aguirre, J. E.

AU - Beelen, A.

AU - Blain, A.

AU - Baker, A. J.

AU - Birkinshaw, M.

AU - Blundell, R.

AU - Bradford, C. M.

AU - Burgarella, D.

AU - Danese, L.

AU - Dunlop, James

AU - Fleuren, S.

AU - Glenn, J.

AU - Harris, A. I.

AU - Kamenetzky, J.

AU - Lupu, R. E.

AU - Maddalena, R. J.

AU - Madore, B. F.

AU - Maloney, P. R.

AU - Matsuhara, H.

AU - Michalowski, Michal

AU - Murphy, E. J.

AU - Naylor, B. J.

AU - Nguyen, H.

AU - Popescu, C.

AU - Rawlings, S.

AU - Rigopoulou, D.

AU - Scott, D.

AU - Scott, K. S.

AU - Seibert, M.

AU - Smail, I.

AU - Tuffs, R. J.

AU - Vieira, J. D.

AU - van der Werf, P. P.

AU - Zmuidzinas, J.

PY - 2010/11/1

Y1 - 2010/11/1

N2 - 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 wide-area submillimeter surveys can simply and easily detect strong gravitational lensing events, with close to 100% efficiency.

AB - 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 wide-area submillimeter surveys can simply and easily detect strong gravitational lensing events, with close to 100% efficiency.

UR - http://www.scopus.com/inward/record.url?scp=78149295965&partnerID=8YFLogxK

U2 - 10.1126/science.1193420

DO - 10.1126/science.1193420

M3 - Article

VL - 330

SP - 800

JO - Science

JF - Science

SN - 0036-8075

ER -

The Detection of a Population of Submillimeter-Bright, Strongly Lensed Galaxies

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