The cooling tail of a long X-ray burst from XTE J1701-407

Bibcode
2008ATel.1618....1L
Linares, M.; Soleri, P.; Curran, P.; Wijnands, R.; Degenaar, N.; van der Klis, M.; Starling, R.; Markwardt, C.
Bibliographical reference

The Astronomer's Telegram, #1618

Advertised on:
7
2008
Number of authors
8
IAC number of authors
0
Citations
7
Refereed citations
2
Description
Swift XRT observed the recently discovered source XTE J1701-407 (Markwardt et al., ATel #1569, Degenaar et al., ATel #1572) on July 17th, 2008 at UT 13:31:45, 97 seconds after the Swift-BAT detection of an X-ray flare (Barthelmy et al., GCN Circ. #7985; Markwardt et al., Atel #1616), for a total exposure time of nearly two kiloseconds. We report herein the analysis of the inital ~1 kilosecond long windowed timing (wt) mode data.
Type
Non-refereed
Gamma-ray bursts
Neutron stars

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