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Fig. 4.

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Visualization of the CMB temperature fluctuation field in the northern hemisphere in two different views. The masked area covers the whole southern hemisphere and the relevant parts of the northern hemisphere, dictated by the PR3 temperature common mask. The visualization is based on the PR3 observed map, cleaned using the SMICA component separation pipeline, degraded at N = 128 and smoothed with a Gaussian kernel of FWHM = 80′.

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