Power spectrum results of the two reconstruction runs. Top row: empirical power spectra calculated directly from the reconstructed sky components (on log10 scale). Bottom row: posterior power spectrum models of the correlated field models representing the τ^c. Left column: angular power spectra. Right column: energy spectrum power spectra. Bold lines show the geometric posterior sample means, while thin lines show individual posterior samples. All power spectra are plotted on log-log scale.