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Table B.1.

Journal listing properties of the observations analyzed in this paper.

Epoch Satellite ObsID (Label) Date Exposure (ks) Rcirc (″) Energy band (keV)
Epoch 1 NuSTAR 90401327002 2018-06-23 32.4 30 3.0-50.0 keV
Swift 00010724012 2018-06-23 2.5 59 0.3-7.0
00010724013 2018-06-23
00010724010 2018-06-23

Epoch 2 NuSTAR 90401327004 2018-07-02 30.0 30 3.0-50.0
Swift 00010724046 2018-07-02 2.5 59 0.3-7.0
00010724047 2018-07-02
00010724048 2018-07-02
00010724049 2018-07-02

Epoch 3 NuSTAR 90401327006 2018-07-14 31.2 30 3.0-30.0
Swift 00088782001 2018-07-14 2.2 35.4 0.3-7.0

Epoch 4 NuSTAR 90401327008 2018-07-22 32.9 30″ 3.0-30.0
Swift 00010724087 2018-07-21 1.6 35.4 0.3-7.0
XMM-Newton 0822580401 2018-07-23 33.0 25 0.3-10.0

Epoch 5 XMM-Newton 0822580501 2018-09-06 45.0 25 0.3-5.0

Epoch 6 XMM-Newton 0822580601 2019-01-20 56.4 25 0.3-1.5

Notes. We group all observations by time into six epochs and fit the data in each epoch simultaneously. Swift observations within the same epoch are combined and treated as a single observation. We also give the radius of the circular region that we use for the source+background spectral extraction in each observation (Rcirc). We followed Evans et al. (2009) in determining the radius of this source+background region to extract for Swift observations. In our spectral analysis, the energy band we use is given in the last column.

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