Fig. C.2.
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The posterior probability distribution of [TBabs*zashift*diskbb] (model 0, left column) and [TBabs*zashift*(diskbb + bbodyrad)] (model 1, central column) applied to the quiescent data for the five epochs of XMM-Newton observation of RX J1301.9+2747. Data are shown for the EPIC-pn camera only and rebinned to 3σ significance. The posterior PDF unconvolved from the instrumental response is plotted for each epoch for the best-fitting model 1 in the right column. The [diskbb] posterior PDF is plotted in dark orange, the [bbodyrad] one in dark yellow, and the total model 1 in gray.
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