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Fig. 7.

image

Evolution of the interstellar absorption NH (panel a), the plasma temperature kT (panel b), the input photon temperature T0 (panel c), the plasma optical depth τp (panel d), and the reduced χ2 of the fits (panel e) as a function of the 1–30 keV flux obtained from the Insight-HXMT spectra using the TBABS × (GAU+CUTOFFPL × GABS) model. Red and blue dots show the same parameters derived from two single NuSTAR observations and two combined observations (NuSTAR+Insight-HXMT), respectively.

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