Fig. A.1.
Spectra and ratio (between the data and model predictions) of ESO 263-13 (XMM-Newton+NuSTAR), UCG 3995B (Chandra+NuSTAR), LEDA 549777 (Swift-XRT+NuSTAR) and NGC 7212 (in M19 sample). NuSTAR and soft X-ray data are plotted in blue and red, respectively. The total best-fit model predictions and different components of the models of are plotted in cyan and black, respectively. The reprocessed component, line-of-sight component, and scattered (and Mekal) component are plotted in dashed, solid, and dotted lines, respectively. Significant flux variabilities are found in ESO 263-13 and UGC 3995B.
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