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

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arxiv 1011.1255 v1 pith:EGF7D5NY submitted 2010-11-04 astro-ph.CO

Mattia Negrello , R. Hopwood , G. De Zotti , A. Cooray , A. Verma , J. Bock , D. T. Frayer , M. A. Gurwell
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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 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. 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
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keywords gravitationalastrophysicaldatagalaxieslargelensingsubmillimeterarea
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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 starforming 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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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Vz-GAL Dusty Star-Forming Galaxies: Revisiting the CO-H2 Conversion Factor Tension

    astro-ph.GA 2026-07 conditional novelty 6.0 of 10

    The CO-to-H2 conversion factor in high-z dusty star-forming galaxies is not required to be 0.8; intermediate to near-Galactic values (median ~4-5) remain dynamically viable.

  2. Strong-lensing Perturber Signatures in Self-interacting Dark Matter Simulations

    astro-ph.CO 2025-10 conditional novelty 6.0 of 10

    Core-collapsed self-interacting dark matter halos in the Concerto simulations reach high enough central densities to match the perturbing masses inferred in J0946, B1938, SDP.81, and SPT2147-50.

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