Swift/XRT observation of H1743-322

Details Swift/XRT observation of H1743-322 Swift/XRT observation of H1743-322

Feb 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008atel.1387....1c&link_type=abstract

The Astronomer's Telegram, #1387

Astronomy and Astrophysics

Astronomy

2

X-Ray, Binaries, Black Holes, Transients

Scientific paper

In order to follow the latest outburst (Atel #1348,#1349,#1352) of the Galactic black hole H1743-322 during its decreasing phase, we asked for a ToO monitoring campaign with Swift/XRT. The first observation lasting 2ks has been performed on 2008, February 12th at 01:31:00 UT. The source has been detected with a 0.1-10 keV count rate of 1.95+/-0.04 counts/s. The best fit is given by an absorbed power law model with a photon index of 1.8+/-0.2 and a column density of 2.4+/-0.3 cm-2.

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