Planck 2013 results
Free Access

Fig. E.2


1D (left) and 2D (right) posterior probability for τ and the combination τAs, for two different Galactic dust templates. These are computed using dust template coefficients estimated with the WMAP “processing” mask. The difference in τ is reduced to ~0.5σ if template coefficients are estimated outside the “P06” Galactic mask.

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