Fig. 3.
Polarization E/B-mode power spectra of radio sources and of dusty galaxies compared with the CMB E mode and B mode for four values of the tensor to scalar ratio r = 0.01, 0.003, 0.001, 0.0003 (from top to bottom); see text and legend for details. Since unresolved point sources on average contribute equally to E and B mode, their total power spectra have been divided by a factor of 2.
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