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Fig. 2
Flux integrated in the joint JEM-X and IBIS/ISGRI range (3.5–60 keV), as derived from the log-parabola spectral fits, vs. a) break energy, as derived from the broken power law fits of time-resolved spectra; b)a index from log-parabola fits; c)b index from log-parabola fits.
This figure is made of several images, please see below:
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