Open Access
Table 1.
Characteristics of the 13 galaxies in the sample.
ID | M* [M⊙] | SFR [M⊙ yr−1] |
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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, is the observed absolute dust-attenuated UV magnitude,
is the intrinsic absolute UV magnitude, fesc(LyC) is the LyC escape fraction, and Mdust is the dust mass.
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