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

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

Jul 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008atel.1618....1l&link_type=abstract

The Astronomer's Telegram, #1618

Astronomy and Astrophysics

Astronomy

6

X-Ray, Binaries, Gamma-Ray Bursts, Neutron Stars, Transients

Scientific paper

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.

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