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; David 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; Daniel Smith; P. Temi; Mark 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; J. S. Dunlop; S. Fleuren; J. Glenn; A.I. Harris; J. Kamenetzky; R. E. Lupu; R. J. Maddalena; B. F. Madore; P. R. Maloney; H. Matsuhara; M. J. Michaowski; 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, David 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, Daniel Smith, P. Temi, Mark 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, J. S. Dunlop, S. Fleuren, J. Glenn, A.I. Harris, J. Kamenetzky, R. E. Lupu, R. J. Maddalena, B. F. Madore, P. R. Maloney, H. Matsuhara, M. J. Michaowski, 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

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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)	800-804
Number of pages	5
Journal	Science
Volume	330
Issue number	6005
DOIs	https://doi.org/10.1126/science.1193420
Publication status	Published - 2010

Keywords

EXTRAGALACTIC SOURCES
REDSHIFT DEADLOCK
STAR-FORMATION
PREDICTIONS
TELESCOPE
EMISSION
CATALOG
COUNTS
QUASAR
FIELD

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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(6005), 800-804. https://doi.org/10.1126/science.1193420

@article{f3933212a6b54a988335856fa289cad6,

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.",

keywords = "EXTRAGALACTIC SOURCES, REDSHIFT DEADLOCK, STAR-FORMATION, PREDICTIONS, TELESCOPE, EMISSION, CATALOG, COUNTS, QUASAR, FIELD",

author = "Mattia Negrello and R. Hopwood and {de Zotti}, G. and A. Cooray and A. Verma and J. Bock and Frayer, {D. T.} and M.A. Gurwell 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, {David G.} and M.J. Jarvis and S. Serjeant and R.J. Ivison and S. Dye and I. Aretxaga and D.H. Hughes 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 C.A. Grady and Clements, {D. L.} and A. Dariush and J. Fritz and D. Hill and J.B. Hornbeck 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 Daniel Smith and P. Temi and Mark Thompson and B.E. Woodgate and D.G. York and J.E. Aguirre and A. Beelen and A. Blain and A.J. Baker and M. Birkinshaw and R. Blundell and C.M. Bradford and D. Burgarella and L. Danese and Dunlop, {J. S.} and S. Fleuren and J. Glenn and A.I. Harris and J. Kamenetzky and Lupu, {R. E.} and Maddalena, {R. J.} and Madore, {B. F.} and Maloney, {P. R.} and H. Matsuhara and Michaowski, {M. J.} and Murphy, {E. J.} and B.J. Naylor and H. Nguyen and C. Popescu and S. Rawlings and D. Rigopoulou and D. Scott and K.S. Scott and M. Seibert and I. Smail and Tuffs, {R. J.} and Vieira, {J. D.} and {van der Werf}, {P. P.} and J. Zmuidzinas",

note = "Original article can be found at : http://www.sciencemag.org/magazine Copyright AAAS. {"}This is the author's version of the work. It is posted here by permission of the AAAS for personal use, not for redistribution. The definitive version was published in Science 330 (6005) pp.800 - 804, doi:http://dx.doi.org/10.1126/science.1193420 {"}",

year = "2010",

doi = "10.1126/science.1193420",

language = "English",

volume = "330",

pages = "800--804",

journal = "Science",

issn = "0036-8075",

publisher = "Springer Nature Link",

number = "6005",

}

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, D, Temi, P, Thompson, M, Woodgate, BE, York, DG, Aguirre, JE, Beelen, A, Blain, A, Baker, AJ, Birkinshaw, M, Blundell, R, Bradford, CM, Burgarella, D, Danese, L, Dunlop, JS, Fleuren, S, Glenn, J, Harris, AI, Kamenetzky, J, Lupu, RE, Maddalena, RJ, Madore, BF, Maloney, PR, Matsuhara, H, Michaowski, MJ, 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, no. 6005, pp. 800-804. 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, David 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, Daniel

AU - Temi, P.

AU - Thompson, Mark

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, J. S.

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 - Michaowski, M. J.

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.

N1 - Original article can be found at : http://www.sciencemag.org/magazine Copyright AAAS. "This is the author's version of the work. It is posted here by permission of the AAAS for personal use, not for redistribution. The definitive version was published in Science 330 (6005) pp.800 - 804, doi:http://dx.doi.org/10.1126/science.1193420 "

PY - 2010

Y1 - 2010

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.

KW - EXTRAGALACTIC SOURCES

KW - REDSHIFT DEADLOCK

KW - STAR-FORMATION

KW - PREDICTIONS

KW - TELESCOPE

KW - EMISSION

KW - CATALOG

KW - COUNTS

KW - QUASAR

KW - FIELD

U2 - 10.1126/science.1193420

DO - 10.1126/science.1193420

M3 - Article

SN - 0036-8075

VL - 330

SP - 800

EP - 804

JO - Science

JF - Science

IS - 6005

ER -

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

Abstract

Keywords

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