Fig. 3
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Histograms of angular alignment deviations according to Eq. (5) in Paper I for filamentary structures. Top left: Planck 857 GHz compared with best fit single-channel H I filaments, all sky. Top right: Planck 857 GHz compared with best fit single-channel H I filaments, |b| > 20°. These two plots were replicated from Fig. 3 in Paper I. Center left: Planck 857 GHz compared with best fit filaments from the VDA velocity field pυ, all sky. Center right: Planck 857 GHz compared with best fit filaments from pυ with |b| > 20°. Bottom left: Planck 857 GHz compared with best fit filaments from the VDA density distribution pd, all sky. Bottom right: Planck 857 GHz compared with best fit filaments from the VDA density distribution pd, |b| > 20°.
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