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
S. Bussmann, R., A. Gurwell, M., Fu, Hai, Smith, Daniel, Dye, S., Auld, R., Baes, M., J. Baker, A., Bonfield, D., Cava, A., L. Clements, D., Cooray, A., Coppin, Kristen, Dannerbauer, H., Dariush, A., De Zotti, G., Dunne, L., Eales, S., Fritz, J., Hopwood, R., Ibar, E., J. Ivison, R., Jarvis, M.J., Kim, S., L. Leeuw, L., Maddox, S., J. Michalowski, M., Negrello, M., Pascale, E., Pohlen, M., A. Riechers, D., Rigby, E., Scott, Douglas, Temi, P., P. Van der Werf, P., Verma, A., Wardlow, J. and Wilner, D.
(2012)
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.
The Astrophysical Journal, 756 (2): 134.
ISSN 0004-637X
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.
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