Swift XRT/UVOT observations of the supersoft X-ray source candidate MAXI J0158-744

Details Swift XRT/UVOT observations of the supersoft X-ray source candidate MAXI J0158-744 Swift XRT/UVOT observations of the supersoft X-ray source candidate MAXI J0158-744

Nov 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011atel.3765....1l&link_type=abstract

The Astronomer's Telegram, #3765

Astronomy and Astrophysics

Astronomy

Optical, Ultra-Violet, X-Ray, Transient

Scientific paper

We report two new Swift follow-up observations of the supersoft source (SSS) candidate MAXI J0158-744 (ATel #3756, #3759). The observations were performed with the XRT on 2011-11-12 17:05:31 UTC and 2011-11-14 01:08:14 UTC for durations of ~2ks each. Both observations were taken in the Window Timing (WT) mode.
Since the detection from MAXI (ATel #3756), the SSS candidate was still bright in X-ray with high count rates of 1.36 ± 0.03 ct/s and 0.34 ± 0.02 ct/s (0.2-2.0 keV) in the 2011-11-12 and the 2011-11-14 WT images, respectively.

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