A Detailed Gravitational Lens Model Based on Submillimeter Array and Keck Adaptive Optics Imaging of a Herschel-ATLAS Sub-millimeter Galaxy at z=4.243

R. S. Bussmann, M. A. Gurwell, Hai Fu, Daniel Smith, S. Dye, R. Auld, M. Baes, A. J. Baker, D. Bonfield, A. Cava, D. L. Clements, A. Cooray, Kristen Coppin, H. Dannerbauer, A. Dariush, G. De Zotti, L. Dunne, S. Eales, J. Fritz, R. HopwoodE. Ibar, R. J. Ivison, M.J. Jarvis, S. Kim, L. L. Leeuw, S. Maddox, M. J. Michalowski, M. Negrello, E. Pascale, M. Pohlen, D. A. Riechers, E. Rigby, Douglas Scott, P. Temi, P. P. Van der Werf, A. Verma, J. Wardlow, D. Wilner

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Abstract

We present high-spatial resolution imaging obtained with the Submillimeter Array (SMA) at 880 μm and the Keck Adaptive Optics (AO) system at KS-band of a gravitationally lensed sub-millimeter galaxy (SMG) at z = 4.243 discovered in the Herschel Astrophysical Terahertz Large Area Survey.
Original languageEnglish
Article number134
Number of pages11
JournalThe Astrophysical Journal
Volume756
Issue number2
DOIs
Publication statusPublished - 10 Sept 2012

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