Fig. 5.
Each subplot shows the data with the folded model in the upper panel and the data-to-model ratio in the lower panel. In the first row, results from the fit of the MCD+PL model are presented, in the second row the DISKPBB model, and, finally, in the third row we have MCD+NTHCOMP. The different columns correspond to Chandra data in the left column, XMM-Newton 2007-05-28 data in the middle column, and 2007-06-19 data in the right column.
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