Late-time observations of the relativistic tidal disruption flare candidate Swift J1112.2-8238
Late-time observations of the relativistic tidal disruption flare candidate Swift J1112.2-8238
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DOI:
10.1093/mnras/stx2193
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发表时间:
2017-08
影响因子:
4.8
通讯作者:
G. C. Brown;A. Levan;E. Stanway;T. Krühler;N. Tanvir;L. Davies;A. Fruchter;S. Cenko;B. Metzger
中科院分区:
文献类型:
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作者:
G. C. Brown;A. Levan;E. Stanway;T. Krühler;N. Tanvir;L. Davies;A. Fruchter;S. Cenko;B. Metzger
GCB thanks the Midlands Physics Alliance for a PhD studentship and the Institute of Advanced Study, Warwick, for postdoctoral research funding. AJL and ERS acknowledge funding from the UK Science and Technology Facilities Council (STFC) associated with grant number ST/L000733/1. TK acknowledges support through the Sofja Kovalevskaja Award to PS from the Alexander von Humboldt Foundation of Germany. We also acknowledge travel funding from the STFC grant ST/M006492/1, and Royal Astronomical Society travel support. Based on observations made with ESO Telescopes at the La Silla Paranal Observatory under programme ID 094.B-0703. Based on observations made with the NASA/ESA HST, obtained at the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-26555. These observations are associated with program 13869. The ATCA is part of the Australia Telescope National Facility which is funded by the Australian government for operation as a national facility managed by CSIRO. The authors made use of the York Extinction Solver (YES, McCall 2004). The authors made use of Ned Wright's Javascript Cosmology Calculator (Wright 2006).