Reasonably good-fit model C for NuSTAR FPMA observation along with its components when reflection ≡ relconv⊗reflionx_hd. Densities for reflection components are iterated to make the fitting consistent from shape as well as flux. The fitted model parameters are presented in Table A.1. Simultaneous NICER observation is also overplotted in the energy range of 0.5-10.0 keV which is sufficient to understand the consistency or inconsistency of reprocessed blackbody in soft X-ray. The best fitted model components turn out to be very similar with the results of model B which is shown in Fig. 3.