Fig. D.4
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Posterior statistics of the M2 thermal dust template modification field for selected energy bins. Top row: Posterior mean of the multiplicative template modification fields on logarithmic color scales. Bottom row: Corresponding posterior multiplicative uncertainty of the modification fields on linear color scales. Energy bins: 1.0–1.78 GeV (left), 10.0–17.8 GeV (middle), and 100–178 GeV (right).
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