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Table 1.

Details of X-ray data analyzed in this paper.

Data set ObsID Date Texp (ks) GTI (ks) Total counts F0.5−10 keV L0.5−10 keV Ref.
[erg s−1 cm−2] [erg s−1]
XMM-01 0111240101 2001-08-06 109.8 70.5/98.2/− 8563/10977/− 2.11 × 10−12 4.45 × 1039 [1]
Suzaku-06 701036010 2006-07-21 108 108/108 27220/7433 4.19 × 10−12 8.45 × 1039 [2]
XMM-13 0701981001 2013-02-03 58.9 37.2/45.6/48.1 39565/15149/18212 8.52 × 10−12 1.80 × 1040 [2],[3]
NuSTAR-13 30002038004 2013-02-03 40.3 40.27/40.21 4353/4179
XMM-14 0656580601 2014-03-01 45.9 23.8/30.4/30.2 5888/2642/1909 3.46 × 10−12 7.30 × 1039
XMM-16 0792382701 2016-08-23 37.0 28.6/5.9/5.0 9712/834/946 3.65 × 10−12 7.70 × 1039
NuSTAR-16 90201034002 2016-08-23 49.8 49.8/49.7 579/750
XMM-18F 0780950201 2018-02-07 45.7 5.7/12.7/20.0 929/863/1413 2.81 × 10−12 5.93 × 1039
XMM-18S 0824450301 2018-09-16 136.2 86.21/114.9/112.4 90239/34360/38045 7.60 × 10−12 1.60 × 1040

Notes. Columns from the left display: name of the data set, observation ID, the date, exposure time, good time intervals (GTI), and net total counts for different detectors, i.e., for XMM-Newton pn/MOS1/MOS2, for Suzaku XIS0+2+3(added)/XIS1, and for NuSTAR FPMA/FPMB. The total counts are given for the following energy ranges: 0.5–10 keV for XMM-Newton and Suzaku, and 3–30 keV for NuSTAR. The unabsorbed flux has been computed using a model composed of diskbb+pl and the luminosity was calculated assuming a distance of 4.2 Mpc. References to the published data are shown in the last column. [1] = First detection of the source by Winter et al. (2006); [2] = First joint XMM-Newton + NuSTAR observation by Walton et al. (2013); [3] = Data fitted by single component model by Różańska et al. (2018).

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