We propose a continuation of the X-ray follow up of GW170817. The main goal of this proposal is to map the late-time behavior of the X-ray emission from GW170817, which will allow us to improve current constraints on the parameters of the merger (jet energetics, off-axis angle, jet structure) and of the environment (density). This is part of our multi- wavelength effort with approved observations in the radio (VLA- ongoing) and HST.
|Effective start/end date||5/7/18 → 5/6/19|
- Smithsonian Astrophysical Observatory (DD8-19101A//NAS8-03060)
- National Aeronautics and Space Administration (DD8-19101A//NAS8-03060)
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