Planck 2018 results
Open Access

Fig. 45.


Power spectra of the difference between the template dust input and output 353 GHz Q maps. The solid blue line shows a random PSM input dust template. The dashed blue line shows the case where the input dust template to SRoll has been taken as the output of the first run. The red curve is obtained by replacing the first ten multipoles in the initial dust template by those of the input sky map.

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