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Fig. 9.
Relation between disk Rin and Tin (i.e., 
in Table 3) obtained from a spectral fitting of diskbb+diskpbb. The relation 
is plotted with a dashed gray line. The blue horizontal dashed lines show various radii for a 10 M⊙ BH. In the case of three fits, Rin is lower than the ISCO for a maximally spinning BH.
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