Fig. B.1.
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X-ray spectra of the AGN detected in the three protocluster. The solid lines are the fit performed using an unabsorbed power law. For sources with more than 30 net counts, the line represents the best fit, while for the other sources (J0819-16, J0819-24, Fab-21, Fab-33, Fab-41) is a power-law with Γ fixed to that found using the HRs.
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