Fig. 12.
Flux of the Gaussian spectral component vs. the flux above 7.11 keV. The circles refer to the first XMM-Newton observation, the triangles refer to during the flare (triangles), and the cross indicates the last XMM-Newton observation. The filled symbols refer to the fluxes derived from NuSTAR best-fit models (see Table A.2). The lines are the linear best fit to the XMM-Newton and NuSTAR data, respectively.
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