Fig.3
Upper panel: all sky map of the dust temperature in K. The temperature is derived from modeling theIRIS100μm and the Planck-HFI emission at 857 and 545 GHz. Lower panel: all sky map of the dust temperature uncertainty in %. The maps are shown in Galactic coordinates with the Galactic centre at the centre of the image. Grey regions correspond to missingIRASdata.
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