Fig. C.1.
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Relation between the error between our work using NuSTAR data and PEXMON model and the error values obtained using PEXRAV and observation from Swift/XRT, Swift/BAT, ASCA, Chandra, and Suzaku by Ricci et al. (2017a). The red circles represent the upper limit of the error bar and the blue stars the lower limit. The dotted black line is x=y.
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