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        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

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        904817.pdf (PDF, 466Kb)
        Author
        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.
        Wilner, D.
        Attention
        2299/9919
        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.
        Publication date
        2012-09-10
        Published in
        The Astrophysical Journal
        Published version
        https://doi.org/10.1088/0004-637X/756/2/134
        Other links
        http://hdl.handle.net/2299/9919
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