Fig. 2.
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Comparison of input maps (first column), reconstructed maps (second column), residual (output minus input) maps (third column), and posterior RMS maps (fourth column) for the baseline SN10 experimental setup. From top to bottom, rows show: (1) Stokes Q CMB in thermodynamic units, (2) Stokes Q synchrotron amplitude at 23 GHz in Rayleigh-Jeans (RJ) units, (3) Stokes Q thermal dust amplitude at 353 GHz in RJ units, (4) synchrotron spectral index, and (5) thermal dust spectral index.
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