Table 3
Derived properties.
| Name | f900,obs | fesc,LyC | fesc,rel,CII | fesc,CII | EW(Lyα) | log ℳH i | log ℳ⋆ | SFR | SSFR | LUV/ |
| 10-15 cgs | % | % | % | [Å] | [ℳ⊙] | [ℳ⊙] | [ℳ⊙ yr-1] | [10-9 yr-1] |
|
|
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) | (11) |
|
|
||||||||||
| Haro 11 | 4.0 ± 0.9 | 3.2 |
8.1 ± 1.2 | 2.4 ± 0.4 | 18.9 | <8.7 | 10.2 | 23.8 | 1.5 | 3.5 |
| VV 114 | <2.1 | <0.4 | 3.9 ± 0.9 | < 0.2 | – | 9.7 | 10.6 | 57.3 | 1.1 | 6.1 |
| MRK 0357 | <2.5 | <2.3 | 4.5 ± 1.1 | < 0.9 | 8.9 | 10.0 | 10.6 | 34.6 | 0.9 | 16.1 |
| SBS 0335-052 | – | – | 16.8 ± 4.9a | 16.8 ± 4.9 | −31.7 | 8.9 | 8.3 | 0.6 | 2.8 | 0.4 |
| Tol 0440-381 | <0.2 | <0.3 | 5.3 ± 1.7 | < 0.6 | 0 | – | 10.0 | 7.7 | 0.8 | 3.9 |
| IRAS 08339+6517 | <4.9 | <6.4 | 3.8 ± 1.3 | 2.8 ± 1.0 | 14.9 | 9.9 | 10.6 | 20.5 | 0.5 | 5.5 |
| NGC 3991 | – | – | 0.0 | 0.0 | 3.2 | 10.6 | 10.0 | 4.1 | 0.4 | 2.4 |
| NGC 4194 | – | – | <4.6 | < 0.1 | 9.2 | 9.4 | 10.3 | 12.1 | 0.6 | 0.5 |
| Tol 1247-232 | 4.4 ± 0.8 | 2.4 |
– | – | 28.6 | – | 9.7 | 27.1 | 5.4 | 12.0 |
| MRK 54 | 1.0 ± 0.7 | 1.2 |
<5.9 | <2.9 | −14.2 | 10.2 | 10.5 | 28.0 | 0.9 | 16.6 |
| MRK 499 | <0.2 | < 0.5 | < 2.5 | < 0.2 | −22.5 | <10.4 | 10.2 | – | – | 1.6 |
| ESO 338-IG04 | – | – | 18.1 ± 1.5 | 16.2 ± 1.3 | 28.3 | 9.1 | 9.1 | 2.5 | 1.7 | 1.6 |
| ESO 185-IG013 | <3.6 | < 16.0 | 12.4 ± 1.8 | 6.0 ± 0.9 | 5.0 | 9.5 | 9.6 | 2.9 | 0.7 | 1.7 |
Notes.(1) The target galaxy; (2) the Lyman continuum flux density [10-15 erg s-1 cm-2 Å-1]; (3) the absolute escape fraction; (4) the relative escape fraction at rest wavelength 1036 Å; (5) the absolute escape fraction estimated from fesc,rel,CII; (6) the Lyα equivalent width; (7) the H i mass; (8) the stellar mass (see Sect. 6 for details); (9) the star formation rate (SFR=SFR(IR)+SFR(UV) (Kennicutt 1998)); (10) the specific star formation rate; (11) the FUV luminosity (The GALEX FUV compared to the local by Wyder et al. 2005).
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