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Fig. 6

image

EBHIS averaged angular power spectrum (black dots) at vLSR = −3.76 km s-1. Systematic and statistical uncertainties are estimated quantitatively by the power spectra calculated for emission free portion of the EBHIS data at vLSR = + 50 km s-1 (green) and vLSR = −200 km s-1 (blue). Data after subtraction of a noise template N(k) are plotted in red. The distribution for k< 0.07 arcmin-1 (vertical line) is approximated by a power-law with γ = −2.86 ± 0.03.

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