Table 2
Measured properties for the 7 galaxies from Gazagnes et al. (2018) without observed Lyman continuum escape fractions.
| Galaxy name | z | EB−V |  |
 |
O32 | |
|---|---|---|---|---|---|---|
| [mag] | [× 10−3] | |||||
| (1) | (2) | (3) | (4) | (5) | (6) | |
| J092600.4+442736a | 0.18069 | 0.11 ± 0.01 | 0.81 ± 0.05 | 50 ± 10 | 3.2 | |
| GP 1244+0216b | 0.23942 | 0.29 ± 0.04 | 0.95 ± 0.13 | 2 ± 1 | 3.2 | |
| GP 1054+5238b | 0.25264 | 0.20 ± 0.04 | 0.89 ± 0.16 | 10 ± 4 | 2.5 | |
| GP 0911+1831b | 0.26223 | 0.35 ± 0.04 | 0.77 ± 0.12 | 4 ± 2 | 1.8 | |
| SGAS J152745.1+065219c | 2.7628 | 0.37 ± 0.002 | 0.99 ± 0.04 | 0.1 ± 0.010 | 1.6 | |
| SGAS J122651.3+215220c | 2.9260 | 0.20 ± 0.001 | 1.00 ± 0.01 | 0.35 ± 0.01 | 1.4 | |
| GP 0303−0759b | 0.16488 | 0.12 ± 0.05 | – | – | 7.3 | |
| J142947.00+064334.9a | 0.1736 | 0.11 ± 0.02 | 0.96 ± 0.06 | 10 ± 1 | – | |
| The Cosmic Eyec | 3.0748 | 0.41 ± 0.01 | 1.00 ± 0.02 | 0.016 ± 0.0005 | – |
Notes. Column 1 gives the galaxy name listed in descending O32 order. Column 2 gives the redshifts of the galaxies. Column 3 is the stellar attenuation (EB−V) measured using the stellar continuum fitting of Paper I. Column 4 is the H I covering fraction measured from the depths of the Lyman series lines (
). Column 5 is the predicted Lyman continuum escape (
) calculated using the Lyman series absorption properties. The sixth column gives the [O III] 5007 Å/[O II] 3727 Å flux ratio (O32). We note that GP 0303−0759, J142947.00+064334.9, and the Cosmic Eye (the three galaxies below the horizontal line) are not included in Sect. 5.3 because GP 0303−0759 does not have a measured
owing to a Milky Way absorption line, and J142947.00+064334.9 and the Cosmic Eye do not have literature O32 values.
References. (a)Heckman et al. (2011,2015); Alexandroff et al. (2015); Heckman & Borthakur (2016). (b) Henry et al. (2015). (c) Wuyts et al. (2012); Rigby et al. (2018).
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