Open Access
Fig. 5.
Q maps power spectra for d, 
, n (all in solid lines), and 
, and cross-spectrum between d1 and d2 (both in dashed lines). This cross-spectrum estimates the power spectrum of the dust emission. Also shown in a solid line is the power spectrum of the GNILC Q map, corresponding to the same Chamaeleon-Musca field.
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