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

Negrello, Mattia; Hopwood, R.; T. Frayer, D.; A. Gurwell, M.; De Zotti, G.; L. Leeuw, L.; Cooray, A.; Verma, A.; Bock, J.; G. Bonfield, D.; Frayer, Dt T.; Gurwell, M. A.; Omont, A.; Neri, R.; Dannerbauer, H.; Leeuw, Ll L.; Jarvis, Mj J.; Barton, E.; Cooke, J.; Kim, S.; da Cunha, E.; J. Jarvis, M.; Rodighiero, G.; J. Ivison, R.; Cox, P.; Bonfield, Dg G.; H. Hughes, D.; Serjeant, S.; Ivison, Rj J.; Dye, S.; Aretxaga, I.; P. Driver, S.; Hughes, Dh H.; Ibar, E.; L. Clements, D.; Bertoldi, F.; Valtchanov, I.; Eales, S.; B. Hornbeck, J.; Dunne, L.; Driver, Sp P.; Auld, R.; E. Rigby, E.; Buttiglione, S.; Cava, A.; Grady, Ca A.; J. B. Smith, D.; Clements, Dl L.; Dariush, A.; A. Thompson, M.; Fritz, J.; Hill, D.; Hornbeck, Jb B.; E. Woodgate, B.; Kelvin, L.; Lagache, G.; Lopez-Caniego, M.; G. York, D.; Gonzalez-Nuevo, J.; Maddox, S.; Pascale, E.; E. Aguirre, J.; Pohlen, M.; Rigby, Ee E.; Robotham, A.; J. Baker, A.; Simpson, C.; Smith, Djb J. B.; M. Bradford, C.; Temi, P.; Thompson, M. A.; S. Dunlop, J.; Woodgate, Be E.; York, Dg G.; Aguirre, Je E.; I. Harris, A.; Beelen, A.; Blain, A.; Baker, Aj J.; E. Lupu, R.; Birkinshaw, M.; Blundell, R.; Bradford, Cm M.; J. Maddalena, R.; Burgarella, D.; Danese, L.; F. Madore, B.; Dunlop, Js S.; Fleuren, S.; Glenn, J.; R. Maloney, P.; Harris, Ai I.; Kamenetzky, J.; Lupu, Re E.; J. Michaowski, M.; Maddalena, Rj J.; Madore, Bf F.; J. Murphy, E.; Maloney, Pr R.; Matsuhara, H.; Michaowski, Mj J.; J. Naylor, B.; Murphy, Ej J.; Naylor, Bj J.; Nguyen, H.; S. Scott, K.; Popescu, C.; Rawlings, S.; Rigopoulou, D.; Scott, D.; J. Tuffs, R.; Scott, Ks S.; Seibert, M.; Smail, I.; D. Vieira, J.; Tuffs, Rj J.; P. Van Der Werf, P.; Vieira, J. D.; van der Werf, P. P.; Pp, van der Werf; Zmuidzinas, J.; Others,

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Giulia Rodighiero
Negrello et al., 2010

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@article{Negrello2010,
  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 = {Negrello, Mattia and Hopwood, R. and T. Frayer, D. and A. Gurwell, M. and De Zotti, G. and L. Leeuw, L. and Cooray, A. and Verma, A. and Bock, J. and G. Bonfield, D. and Frayer, Dt T. and Gurwell, M. A. and Omont, A. and Neri, R. and Dannerbauer, H. and Leeuw, Ll L. and Jarvis, Mj J. and Barton, E. and Cooke, J. and Kim, S. and da Cunha, E. and J. Jarvis, M. and Rodighiero, G. and J. Ivison, R. and Cox, P. and Bonfield, Dg G. and H. Hughes, D. and Serjeant, S. and Ivison, Rj J. and Dye, S. and Aretxaga, I. and P. Driver, S. and Hughes, Dh H. and Ibar, E. and L. Clements, D. and Bertoldi, F. and Valtchanov, I. and Eales, S. and B. Hornbeck, J. and Dunne, L. and Driver, Sp P. and Auld, R. and E. Rigby, E. and Buttiglione, S. and Cava, A. and Grady, Ca A. and J. B. Smith, D. and Clements, Dl L. and Dariush, A. and A. Thompson, M. and Fritz, J. and Hill, D. and Hornbeck, Jb B. and E. Woodgate, B. and Kelvin, L. and Lagache, G. and Lopez-Caniego, M. and G. York, D. and Gonzalez-Nuevo, J. and Maddox, S. and Pascale, E. and E. Aguirre, J. and Pohlen, M. and Rigby, Ee E. and Robotham, A. and J. Baker, A. and Simpson, C. and Smith, Djb J. B. and M. Bradford, C. and Temi, P. and Thompson, M. A. and S. Dunlop, J. and Woodgate, Be E. and York, Dg G. and Aguirre, Je E. and I. Harris, A. and Beelen, A. and Blain, A. and Baker, Aj J. and E. Lupu, R. and Birkinshaw, M. and Blundell, R. and Bradford, Cm M. and J. Maddalena, R. and Burgarella, D. and Danese, L. and F. Madore, B. and Dunlop, Js S. and Fleuren, S. and Glenn, J. and R. Maloney, P. and Harris, Ai I. and Kamenetzky, J. and Lupu, Re E. and J. Michaowski, M. and Maddalena, Rj J. and Madore, Bf F. and J. Murphy, E. and Maloney, Pr R. and Matsuhara, H. and Michaowski, Mj J. and J. Naylor, B. and Murphy, Ej J. and Naylor, Bj J. and Nguyen, H. and S. Scott, K. and Popescu, C. and Rawlings, S. and Rigopoulou, D. and Scott, D. and J. Tuffs, R. and Scott, Ks S. and Seibert, M. and Smail, I. and D. Vieira, J. and Tuffs, Rj J. and P. Van Der Werf, P. and Vieira, J. D. and van der Werf, P. P. and Pp, van der Werf and Zmuidzinas, J. and Others, },
  doi = {10.1126/science.1193420},
  month = {nov},
  title = {The detection of a population of submillimeter-bright, strongly lensed galaxies},
  url = {https://www.researchgate.net/profile/Steve_Maddox/publication/47679209_The_Detection_of_a_Population_of_Submillimeter-Bright_Strongly_Lensed_Galaxies/links/0fcfd5064ccf613264000000.pdf},
  year = {2010}
}

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

Journal article published in 2010 by Mattia Negrello, R. Hopwood, D. T. Frayer, M. A. Gurwell, G. De Zotti, L. L. Leeuw, A. Cooray, A. Verma, J. Bock, D. G. Bonfield, Dt T. Frayer, M. A. Gurwell, A. Omont, R. Neri, H. Dannerbauer and other authors. Mattia Negrello, R. Hopwood, D. T. Frayer, M. A. Gurwell, G. De Zotti, L. L. Leeuw, A. Cooray, A. Verma, J. Bock, D. G. Bonfield, Dt T. Frayer, M. A. Gurwell, A. Omont, R. Neri, H. Dannerbauer, Ll L. Leeuw, Mj J. Jarvis, E. Barton, J. Cooke, S. Kim, E. da Cunha, M. J. Jarvis, G. Rodighiero

, R. J. Ivison, P. Cox, Dg G. Bonfield, D. H. Hughes, S. Serjeant, Rj J. Ivison, S. Dye

, I. Aretxaga, S. P. Driver, Dh H. Hughes, E. Ibar, D. L. Clements, F. Bertoldi, I. Valtchanov, S. Eales, J. B. Hornbeck, L. Dunne, Sp P. Driver

, R. Auld, E. E. Rigby, S. Buttiglione, A. Cava, Ca A. Grady, D. J. B. Smith, Dl L. Clements, A. Dariush, M. A. Thompson, J. Fritz, D. Hill, Jb B. Hornbeck, B. E. Woodgate, L. Kelvin, G. Lagache, M. Lopez-Caniego, D. G. York, J. Gonzalez-Nuevo, S. Maddox

, E. Pascale, J. E. Aguirre, M. Pohlen, Ee E. Rigby, A. Robotham, A. J. Baker, C. Simpson, Djb J. B. Smith

, C. M. Bradford, P. Temi, M. A. Thompson, J. S. Dunlop, Be E. Woodgate, Dg G. York, Je E. Aguirre, A. I. Harris, A. Beelen, A. Blain, Aj J. Baker, R. E. Lupu, M. Birkinshaw, R. Blundell, Cm M. Bradford, R. J. Maddalena, D. Burgarella, L. Danese, B. F. Madore, Js S. Dunlop, S. Fleuren, J. Glenn, P. R. Maloney, Ai I. Harris, J. Kamenetzky, Re E. Lupu, M. J. Michaowski, Rj J. Maddalena, Bf F. Madore, E. J. Murphy, Pr R. Maloney, H. Matsuhara, Mj J. Michaowski, B. J. Naylor, Ej J. Murphy, Bj J. Naylor, H. Nguyen, K. S. Scott, C. Popescu, S. Rawlings, D. Rigopoulou, D. Scott, R. J. Tuffs, Ks S. Scott, M. Seibert, I. Smail

, J. D. Vieira, Rj J. Tuffs, P. P. Van Der Werf, J. D. Vieira, P. P. van der Werf, van der Werf Pp, J. Zmuidzinas, Others

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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.

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

Abstract