TRIShUL: Technique for Reconstructing magnetic Interstellar Structure Using starLight polarization

Open Access

Fig. D.1

Distribution of FN decomposition results for 1200 two-cloud mock samples using TRIShUL. The statistics represents the resulted FN for five random samples of input combination of background star fraction (f_bg2, separate panels), maximum polarization of second cloud ( $p_{i n p u t}^{(2)}$ $p_{\rm{input}}^{(2)}$ , along X-axis), and differential polarization angle between two clouds (ψ, Y-axis).

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