Table B.1.
Overview of some studies of individual LyC leakers at high redshift. The subscript rel. means relative escape fraction, abs. means absolute. If the information is not given in the subscript it is not clear from the paper. It has to be noted though that the definition of escape fraction also is not uniform, which explains some of the discrepancies.
| object(s) | paper(s) | redshift | fesc, LyC | notes |
|---|---|---|---|---|
| C49 | Shapley et al. (2006), Siana et al. (2015) | z = 3.15 | fesc, rel = 65% | in the field SSA 22a, but reexamined by Siana et al. (2015) (foreground contamination) |
| D3 | Shapley et al. (2006) | z = 3.07 | fesc, rel ≥ 100% | in the field SSA 22a |
| Ion1 | Vanzella et al. (2010a), Vanzella et al. (2012), Vanzella et al. (2015), Vanzella et al. (2020), Ji et al. (2020) | z = 3.794 | fesc, abs = 5 ± 2%, fesc, rel = 32 ± 11% | from Ji et al. (2020), who also stack 107 galaxies but find no LyC signal |
| Ion2 | Vanzella et al. (2015), Vanzella et al. (2016), de Barros et al. (2016), Vanzella et al. (2020) | z = 3.212 |
 |
from de Barros et al. 2016 |
| Ion3 | Vanzella et al. (2018) | z = 4.0 | fesc, rel ≈ 60% | |
| MD5b | Mostardi et al. (2015) | z ≈ 3.14 | fesc, rel = 75 − 100% | follow-up of Mostardi et al. (2013) |
| Q1549-C25 | Shapley et al. (2016) | z = 3.15 | fesc, abs > 51% | |
| Horseshoe | Vasei et al. (2016) | z = 2.38 | fesc, rel < 0.08 | non detection in lensed galaxy |
| A2218-Flanking | Bian et al. (2017) | z = 2.5 | fesc, abs > 28 − 57% | |
| GN-UVC-6 | Jones et al. (2018) | z = 2.439 | 6 candidates, one AGN, 4 contaminations | |
| Sunburst arc | Rivera-Thorsen et al. (2017a), Rivera-Thorsen et al. (2019), Vanzella et al. (2020), Mainali et al. (2022) | z = 2.37 |
 |
lensed, values from Rivera-Thorsen et al. (2019) |
| AUDFs01 | Saha et al. (2020) | z = 1.42 | fesc, rel > 20% | observed with AstroSat, near the peak of star formation |
| J0121+0025 | Marques-Chaves et al. (2021) | z = 3.244 | fesc, abs ≈ 40% | very luminous with a young star burst |
| J1316-2614 | Marques-Chaves et al. (2022) | z = 3.613 | fesc, abs ≈ 90% | UV-bright starburst |
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