The SPHINX public data release - II. Using low-ionisation absorption lines and dust attenuation to predict Lyman continuum escape

Open Access

Fig. 8.

Comparison of Equation (7) applied to LzLCS residual fluxes and dust attenuations (x-axis) with $f_{esc}^{900}$ $Mathematical equation: $ {f_{\mathrm{esc}}^{900}} $$ estimated in Flury et al. (2022a) with the UV SED f_esc method (y-axis). The yellow points correspond to galaxies from the LzLCS survey itself, while the green points correspond to leakers detected earlier (Izotov et al. 2016a,b, 2018, 2021; Wang et al. 2019). The upper limits are indicated with open symbols and downward arrows.

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