Fig. 34
T–T plots between the polarization and AME intensities (both in units of μK at 22.8 GHz). Top: Perseus; bottom: Pegasus plume. The scatter is mostly due to thermal noise in the polarization map (uncertainties in the polarization intensity in these regions are typically around 5 μK). The fitted slope gives the polarization fraction for the region, based on the linear fit (dashed line).
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