Fig. 14
The black continuous line with the crosses and bold error bars show the power spectrum of IRIS 100 μm and the red dotted line with squares and thin error bars represents the power spectrum of the emission of the cirrus at 100 μm calculated from the Hi map. The discrepancy observed for k > 0.02 arcmin-1 is due to the clustering of SB galaxies (see Sect. 6.2).
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