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Table C.5.

Swift/XRT observation log and spectral fit results for IGR J17503−2636.

Sequence MJD Start time (UT) End time (UT) Exposure NH Γ F0.3 − 10 keV Cstat/d.o.f.
00010980001 58576.71546 2019-04-03 17:10:15 2019-04-03 22:17:53 5178 120.2/142
00010980002 58583.49265 2019-04-10 11:49:25 2019-04-10 15:26:52 3372 83.9/116
00010980003 58590.53303 2019-04-17 12:47:33 2019-04-17 20:56:53 4944 95.2/79
00010980005 58611.77889 2019-05-08 18:41:35 2019-05-08 22:20:52 4012 229.8/278
00010980006 58618.10236 2019-05-15 02:27:23 2019-05-15 15:10:53 4897 216.9/279
00010980007 58643.79713 2019-06-09 19:07:51 2019-06-10 00:06:53 4734 219.1/269
00010807001 58343.82179 2018-08-13 19:43:22 2018-08-13 20:13:11 990 118.2/156
00088805001 58353.19412 2018-08-23 04:39:32 2018-08-23 06:38:52 1858 70.0/82
00048022007 56224.21009 2012-10-24 05:02:31 2012-10-24 05:30:54 1702 44.4/47

Notes. We show: observing sequence, date (MJD of the middle of the observation), start and end times (UT), and XRT exposure time in seconds. We also report the absorption column density NH in units of 1023 cm−2, the powerlaw photon index Γ, and the flux in the 0.3–10 keV energy band (not corrected for absorption in units of 10−11 erg cm−2 s−1) as determined from the spectral fit.

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