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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