Fig. 11.

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Fitting outcomes derived from the TBabs×zxipcf×edge×edge×nthComp model (Model 3). Illustrating the evolution of neutral hydrogen absorption nH from the interstellar medium (ISM) and cold dust. It further details the wind column density Nh, the degree of wind ionization represented by log (ξ), the photon index Γ, the seed photon temperature kTbb, and the luminosity before absorption. Within the zxipcf component, the covering fraction and redshift are held constant at values of 1 and 0, respectively. From the joint fitting results, the electron temperature kTe in the nthComp model remains fixed at 4 keV.
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