Fig. 6
γ-ray detection efficiency for each bin in FOM. Red represents the 2WHSP-FGL subsample (2WHSP sources with FGL counterparts: 439 objects), and blue the 2WHSP* subsample (2WHSP sources considering all 150 new + 439 FGL γ-ray counterparts). The first bin at FOM = 1.2 condensate all cases with FOM > 1.2 (sources with the brightest synchrotron peak flux −11.2 < Log(νpeakfνpeak) <−9.7) since almost all of them have been already γ-ray detected, having a 3FGL counterpart.
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