Fig. 13
Distribution of synchrotron peak fluxes for the 1WHSP sources that have been detected so far (bottom panel) and that are still undetected in the TeV band (top panel). For each bin in νpeakFνpeak we report the percentage of 1WHSP sources that are already TeV detected. Central and left dashed lines correspond respectively to the detectability limit of present Cherenkov Telescopes and approximately to the future CTA.
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