Fig. 1
Composite three-colour image showing Herschel/SPIRE intensities for the region considered, where available (with the 250 μm; 350 μm; 500 μm bands shown in blue, green, and red). For regions outside the Herschel coverage, we used the Planck/IRAS dust model (τ850, T, β) to predict the intensity that would be observed at the SPIRE passbands. Toggle labels
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