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Table 3.

Investigating the impact of different dust extinction assumptions in J1154+2443 and J1256+4509.

Galaxy name Law EB − V Age Cf(H I) A(LyC) A(Lyα) WSS
[Myr]
(1) (2) (3) (4) (5) (6) (7) (8) (9)
J1154+2443 0.46 Reddy+16 0.118 ± 0.031 8.10 0.401 ± 0.152 1.51 1.20 733
0.00 ( * ) 15.07 0.379 ± 0.145 0.00 0.00 770
0.20 ( * ) 4.20 0.339 ± 0.183 2.57 2.04 743
SMC 0.034 ± 0.008 7.99 0.483 ± 0.390 0.87 0.55 733
J1256+4509 0.38 Reddy+16 0.076 ± 0.029 2.52 0.408 ± 0.125 0.98 0.78 1517
0.00 ( * ) 3.15 0.440 ± 0.121 0.00 0.00 1555
0.20 ( * ) 2.32 0.571 ± 0.183 2.57 2.04 1518
SMC 0.038 ± 0.008 2.38 0.383 ± 0.133 0.98 0.62 1499

Notes. (1) Galaxy name; (2) observed LyC escape fraction; (3) dust attenuation law; (4) dust extinction; (5) light-weighted stellar continuum age from the fit, derived from the linear combination of the 50 single-age STARBURST99 stellar continuum; (6) H I covering fraction value and uncertainty returned by the fit; (7) Attenuation at 912 Å; (8) Attenuation at 1216 Å and (9) the value of the summed squared weighted residuals for the returned parameter values as given by MPFIT. ( * )Values fixed during the fitting procedure.

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