Planck early results
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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.

This figure is made of several images, please see below:

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