zELDA II: Reconstruction of galactic Lyman-alpha spectra attenuated by the intergalactic medium using neural networks

Open Access

Fig. G.1

Left: $f_{esc}^{4 \overset{\circ}{A}}$ $f_{\text{esc}}^{4\ {\mathop{\mathrm{A}}^{\circ}}}$ distribution as a function of redshift in the REC+z model. The solid line shows the 50 percentile, while, from darker to lighter, the shadows show the 1σ, 2σ and 3σ. Right: Same as as Fig. 6 but for REC+z at S/N_p = 15.0 and W_in = 0.1 Å.

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