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Fig. 5.


Wavelet planes of different Galactic neighbourhoods along the zero-azimuth line. Panels ai: correspond to the volumes V1–V9 described in Table 1. We show the coefficients in a common colour bar with the significant peaks superposed and contours in the same manner as in Fig. 2. We notice the change in colour caused by the difference in number of stars of each subsample. Also, for the SN sample, the most crowded regions of the plane saturate (cf. Fig. 4).

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