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Table 1.

Characteristics of the 13 galaxies in the sample.

ID M* [M] SFR [M yr−1] M UV obs $ M_{\mathrm{UV}}^{\mathrm{obs}} $ M UV intr $ M_{\mathrm{UV}}^{\mathrm{intr}} $ fesc(LyC) Mdust [M]
2899 1.4 × 1010 31.0 −19.4 −21.5 0.001 1.1 × 107
24688 6.4 × 109 35.7 −19.4 −23.4 0.004 8.7 × 106
55468 4.9 × 109 17.9 −19.0 −21.9 0.002 9.8 × 106
36112 3.7 × 109 22.8 −19.4 −22.3 0.007 1.4 × 107
41163 3.2 × 109 8.4 −19.0 −21.9 0.007 5.5 × 106
3639 2.6 × 109 18.1 −19.1 −21.8 0.001 5.9 × 106
42655 1.7 × 109 10.0 −19.2 −21.5 0.023 5.8 × 106
8776 1.6 × 109 6.2 −19.0 −20.9 0.026 8.3 × 106
39021 1.5 × 109 9.5 −19.0 −21.1 0.033 8.0 × 106
76168 1.5 × 109 8.0 −19.2 −21.6 0.011 3.1 × 106
10345 2.5 × 108 1.5 −19.1 −20.0 0.235 1.5 × 106
57172 2.4 × 108 1.5 −19.3 −19.8 0.485 1.2 × 106
67244 7.0 × 107 0.7 −19.0 −19.4 0.195 2.1 × 105

Notes. Here, M* is their stellar mass, SFR is the star formation rate, calculated over 10 Myr, M UV obs $ M_{\mathrm{UV}}^{\mathrm{obs}} $ is the observed absolute dust-attenuated UV magnitude, M UV intr $ M_{\mathrm{UV}}^{\mathrm{intr}} $ is the intrinsic absolute UV magnitude, fesc(LyC) is the LyC escape fraction, and Mdust is the dust mass.

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