Statistical description of dust polarized emission from the diffuse interstellar medium - A RWST approach

B. Regaldo-Saint Blancard; F. Levrier; E. Allys; E. Bellomi; F. Boulanger

doi:10.1051/0004-6361/202038044

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Volume 642 (October 2020)

A&A, 642 (2020) A217

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Fig. C.4

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(left column), (middle column) and (right column) RWST coefficients for the data set. In the plot, each curve corresponds to a fixed j₁ value while j₂ ranges from j₁ + 1 to J − 1 = 6. For j₁ = J − 2, the curve is reduced to a single dot on the figure.

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