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Table B.2.

Overview of some of the currently known LyC emission at high redshift, showing results from surveys or stacks, often using star-forming galaxies (SFGs), AGN, LAEs or LBGs.

object(s) paper(s) redshift fesc, LyC notes
29 LBGs Steidel et al. (2001) z = 3.4 fesc ≳ 50 5 times more LyC photons per unit comoving volume compared to quasars at z≈3

14 SFGs Shapley et al. (2006) z ≈ 3 fesc = 14

7/73 LBGs, 10/125 LAEs Iwata et al. (2009) z ≃ 3.1 fesc, rel = 0.45

102 LBGs Vanzella et al. (2010a) z = 3.4 − 4.5 they also find one individual candidate

15 starburst galaxies Siana et al. (2010) z ≈ 1.3 fesc, rel < 0.02 stacked limit, 3σ

11 LBGs Boutsia et al. (2011) z ≈ 3.3 fesc, rel < 5% smallest limit at that z

6/26 LBGs, 28/130 LAEs Nestor et al. (2011) z ≈ 3 ∼10% for LBGs low UV/LyC ratios of LAEs explained with orientation effects, follow-up of SSA22 field

9/41 LBGs, 20/91 LAEs Nestor et al. (2013) z ≈ 3 , follow-up of SSA22 field

4/49 LBGs, 7/91 LAEs Mostardi et al. (2013) z ≈ 2.85 ,

∼600 SFGs Rutkowski et al. (2016) z ≈ 1 fesc, abs < 2.1% 3σ limit from individual non-detections

37 galaxies Grazian et al. (2016) z ≈ 3.3 fesc, rel < 2% two individual detections, fesc for stacks

7 lensed galaxies Leethochawalit et al. (2016) 4 < z < 5 fesc, abs ≃ 19 ± 6%

588 Hα galaxies, 160 LAEs Matthee et al. (2017) z ≈ 2 fesc < 2.8 (6.4)% stacking median (mean)

69 SFGs Grazian et al. (2017) z ≈ 3.3 ,

SFGs Rutkowski et al. (2017) z ≈ 2.5 fesc, rel < 15% selected on [OII] and high [OIII]/[OII]

6 galaxies Naidu et al. (2017) z ≈ 2 fesc > 60%

73 galaxies Naidu et al. (2018) z ≈ 3.5 selected based on high [OIII]/[OII] but no LyC detection

124 galaxies Steidel et al. (2018) z ≈ 3 fesc, abs = 0.09 ± 0.01

61 galaxies Fletcher et al. (2019) z ≃ 3.1 20% of objects show LyC leakage

110 galaxies Smith et al. (2020) 2.26 < z < 4.3 dominated by AGN

5 candidates Jones et al. (2021) 2.35 < z < 3.05

11 candidates Saxena et al. (2022) 3.1 < z < 3.5 fesc, abs = 0.7 − 0.52

6 candidates Rivera-Thorsen et al. (2022) 2 < z < 3.5 fesc, abs = 0.36 − 1

148 SFGs Begley et al. (2022) z ≃ 3.5 fesc = 0.07 ± 0.02

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