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Fig. 11
Mask used for the AME T–T plots. The regions in grey are masked in the T–T plots. The region in light blue shows where the AME at 22.8 GHz is brighter than 1 mK; this is also masked when determining the best-fitting emissivity. We also mask the ecliptic plane (| β | < 20deg) when analysing the IRAS and WISE data.
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