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Fig. B.1


Average (solid lines) and rms (shaded areas) of φp(10 − 100   GeV) (upper panel), TS (middle panel), and the scaling h(θs) (lower panel) as function of the intrinsic angular extent θs. For each θs, a sample of 500 simulations of the 1FGL J0030.7+0724 photon distribution between 10 and 100 GeV assuming a DM subhalo intensity profile was analysed with the 1FGL point-source-analysis framework.

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