Fig. 3.
Left and middle panels: flux-resolved EPIC-pn spectra of RX J1301.9+2747 in the 2000 and 2019 observations, along with spectral residuals to model 3. Right panel: model 3; the dashed line is the power law, the dotted line the disk blackbody (both kept tied within the low-flux and high-flux state of each observation), and the dashed-dotted line the bremsstrahlung emission emerging in the high-flux spectra.
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