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Fig. E.2.

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Influence of BP/X-shaped structures and dark matter halos on model results. The top panels show the marginalised chi-squares χnorm2 = (χ2 − χmin2)/ΔχCL2 versus model-recovered bar pattern speeds Ωp, while the bottom panels display χnorm2 versus model-recovered bar azimuthal angles φ. Left panels correspond to the results of Au-23-85-50 and right panels are for Au-23-85-80. Each fold line represents a complete set of modelling runs. The black fold lines denote the default model results, which incorporate BP/X-shaped structures and allow dark matter halos to vary freely, as previously displayed in the middle panel of Fig. 7. The blue lines correspond to results with constrained dark matter halos, requiring the differences between model-recovered and true dark matter mass within 10 kpc to be less than 10% ( 0.9 M dm , 10 kpc true < M dm , 10 kpc model < 1.1 M dm , 10 kpc true $ 0.9M_{\mathrm{dm,10kpc}}^{\mathrm{true}} < M_{\mathrm{dm,10kpc}}^{\mathrm{model}} < 1.1M_{\mathrm{dm,10kpc}}^{\mathrm{true}} $). The red lines represent the results ignoring BP/X-shaped structures. The horizontal dashed lines represent 1σ (68%, χnorm2 = 1) and 2σ (95%, χnorm2 = 2) confidence levels. The vertical dotted lines denote the true bar pattern speeds ΩT or azimuthal angles φT, with their values shown by the green annotations.

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