The Impact of Polarized Extragalactic Radio Sources on the Detection of CMB Anisotropies in Polarization
Figure 7
Polarization power spectra at six Planck frequencies for the CMB radiation (black lines: dotted lines for the E-mode; solid lines for the gravitational wave B-mode with , 0.01 and 0.001; dashed lines for the lensing-induced B-mode) and for ERS (solid lines are for Jy and dashed lines for Jy; blue lines correspond to the more “conservative” case and red lines to the more “optimistic” case).
