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Fig. 4.

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Lyα observables (top panel: LLyα; middle panel: EWLyα; bottom panel: f esc Lyα $ {f^\mathrm{Ly\alpha}_\mathrm{esc}} $ ) vs. galaxy inclination. Filled purple symbols are based on the kinematical inclination, i, from the disc modelling of the RDs with GalPak3D. Unfilled symbols are based on photometric inclinations (purple: RD; green: PR) according to cos(i)≈(b/a)I, where (b/a)I is the I-band axis ratio from Rasekh et al. (2022). Thus, each RD is represented by a filled and an open symbol in these plots. Circles with error bars indicate measurements of the Lyα observables, whereas downward-pointing triangles indicate upper limits. Correlation coefficients (Kendall’s τ) and corresponding p-values for the kinematical inclinations are provided in the top-right corner of each panel.

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