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Fig. 2
Effective beam FWHM of the GNILC dust maps on the whole sky (top panel) and on a 
area of the sky centred at high latitude (l,b) = (90°,−80°) (bottom panel). The spatially varying beam FWHM is the same for all frequencies. GNILC preserves the 5′-scale power of the thermal dust in the high signal-to-noise regions of the sky.
This figure is made of several images, please see below:
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