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Fig. 14.

image

Panel A: photon index Γw vs. flux (0.3–2 keV) of the warm NTHCOMP component, for the different observations. Panel B: primary X-ray flux (3–10 keV) of the hot NTHCOMP component vs. flux of the warm NTHCOMP component. The fluxes are in units of 10−11 erg s−1 cm−2. Red dashed lines represent linear fits to the data.

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