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Table 3

Results of power-law fits to the power spectra computed on simulated dust maps for the six Galactic regions from PXXX.

0.24 0.33 0.42 0.53 0.63 0.72

AEE(μK2) 30.6±2.3 50.4±2.8 95.2±4.9 157.6±7.7 261±12 419±20
α EE 2.37±0.13 2.307±0.099 2.438±0.092 2.334±0.087 2.385±0.084 − 2.413±0.088
r Aα,E − 0.85 0.84 − 0.83 − 0.83 − 0.82 − 0.81
χ2(Nd.o.f. = 5) 0.1 0.7 0.4 0.8 1.4 1.0

ABB(μK2) 14.3±1.1 24.7±1.5 44.9±2.4 74.0±4.0 123.6±6.4 196±11
α BB 2.35±0.14 2.33±0.11 2.439±0.099 2.313±0.098 2.332±0.094 2.40±0.10
r Aα,B 0.82 0.82 0.81 0.81 0.81 0.81
χ2(Nd.o.f. = 5) 0.6 0.1 0.7 0.9 0.5 1.4

AEE,data(μK2) 37.5±1.6 51.0±1.6 78.6±1.7 124.2±1.9 197.1±2.3 328.0±2.8
2.40±0.09 2.38±0.07 2.34±0.04 2.36±0.03 2.42±0.02 2.43±0.02

ABB,data(μK2) 18.4±1.7 24.5±1.7 41.7±1.8 67.1±2.7 104.5±2.3 173.8±3.6
2.29±0.15 2.37±0.12 2.46±0.07 2.43±0.05 2.44±0.03 2.46±0.02

Notes. The quantities rAα,X and χ2 are the correlation between AXX and αXX and the value of the χ2 at the fit values, respectively. Values from the Planck data taken from PXXX are given for comparison.

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