Fig. 45
Amplitude ratio between total polarized foregrounds and CMB as a function of both multipole moment and frequency, defined by 
, as defined Eq. (22) with parameters derived from 73% of the sky. The left and right panels show the EE and BB spectra, and the black and red contours in the latter corresponds to tensor-to-scalar ratios of r = 0.0 and 0.05, respectively.
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