Fig. 3
Best-fit power-law exponents αEE (red squares)
and αBB (blue
circles) fitted to the 353 GHz dust 
and
power spectra for the different LR
regions defined in Sect. 3.3.1, distinguished
here with fsky. Although the values in the
regions are not quite independent, simple means have been calculated and are
represented as red and blue dashed lines.
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