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Fig. 6

image

SEDsfitting results assuming a synchrotron origin of the X-ray emission. The curves represent the best-fit models. Forknots D, B, and C both a broken power-law fit and a fit based on two exponential cut-off power-law components (dashed and dot-dashed curves, with superposition corresponding to the solid curve) assuming β = 1 are shown. The X-ray flux densities from Marshall et al. (2002) are also plotted for comparison (grey symbols).

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