Fig. 14
Left panel: scatter plot of
Scls vs. 
.
For each source in our 2FGLTS>16 list, associated to one or more
γ-ray DBSCAN cluster, we plot the
in the 3–10 GeV band vs. the average values of Scls and
its standard deviation (represented by the error bar). Right panel:
the distribution (blue line) of the square of the significance for the fake
clusters in the Fermi-LAT real sky for the full
K, ε parameter space compared to a
χ2 distribution with one degree of freedom.
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