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Fig. 14
Phase fractions for CNM dominated regions depending on the width of the smoothing kernel used for the generation of the mask. Top panel: high latitudes |b| > 20° only, bottom panel: all sky data. From left to right: phase fractions for |vLSR| < 8, |vLSR | < 4, and |vLSR| < 1 km s−1 are shown.
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