The detection of a population of submillimeter-bright, strongly lensed galaxies.
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, i...
المؤلفون الرئيسيون: | Negrello, M, Hopwood, R, De Zotti, G, Cooray, A, Verma, A, Bock, J, Frayer, D, Gurwell, M, Omont, A, Neri, R, Dannerbauer, H, Leeuw, L, Barton, E, Cooke, J, Kim, S, da Cunha, E, Rodighiero, G, Cox, P, Bonfield, D, Jarvis, M, Serjeant, S, Ivison, R, Dye, S, Aretxaga, I, Hughes, D |
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التنسيق: | Journal article |
اللغة: | English |
منشور في: |
2010
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مواد مشابهة
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The detection of a population of submillimeter-bright, strongly lensed galaxies
حسب: Negrello, M, وآخرون
منشور في: (2010) -
Spitzer imaging of Herschel-atlas gravitationally lensed submillimeter sources
حسب: Hopwood, R, وآخرون
منشور في: (2011) -
SPITZER IMAGING OF HERSCHEL-ATLAS GRAVITATIONALLY LENSED SUBMILLIMETER SOURCES
حسب: Hopwood, R, وآخرون
منشور في: (2011) -
A DETAILED GRAVITATIONAL LENS MODEL BASED ON SUBMILLIMETER ARRAY AND KECK ADAPTIVE OPTICS IMAGING OF A HERSCHEL-ATLAS SUBMILLIMETER GALAXY AT z=4.243
حسب: Bussmann, R, وآخرون
منشور في: (2012) -
Green Bank Telescope Zpectrometer CO(1-0) observations of the strongly lensed submillimeter galaxies From the Herschel ATLAS
حسب: Frayer, D, وآخرون
منشور في: (2011)