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Fig. 4.

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Directional analysis of the GRBs fluence: masked case. Left panel: distribution of GRB on the celestial sphere of the FERMIGRB masked sample, showing 2428 GRBs, where we implemented a cut of the zone of avoidance removing GRBs with |b|≤20° (in Galactic coordinates). Middle and Right panels: f FERMI MKD $ f^{\mathrm{FERMI}_{\mathrm{MKD}}} $-map with resolution Nside = 4 (middle panel) and its dipole component (right panel) for the FERMIGRB-Masked sample. All the maps are in units of erg/cm2 and in the Galactic coordinate system.

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