Table 1
Sample of galaxies with Lyman series observations.
Galaxy name | z | 12 + log (O/H) | ![]() |
R |
---|---|---|---|---|
(1) | (2) | (3) | (4) | (5) |
J0921+4509 | 0.23499 | 8.67a | 0.010g | 15 000 |
J1503+3644 | 0.3537 | 7.95b | 0.058b | 1500 |
J0925+1409 | 0.3013 | 7.91c | 0.072c | 1500 |
J1152+3400 | 0.3419 | 8.00b | 0.132b | 1500 |
J1333+6246 | 0.3181 | 7.76b | 0.056b | 1500 |
J1442–0209 | 0.2937 | 7.93b | 0.074b | 1500 |
Tol1247–232 | 0.0482 | 8.10d | 0.004h | 1500 |
Tol0440–381 | 0.0410 | 8.20d | 0.019h | 1500 |
Mrk54 | 0.0451 | 8.60d | <0.002h | 1500 |
J0926+4427 | 0.18069 | 8.01e | – | 15 000 |
J1429+0643 | 0.1736 | 8.20e | – | 15 000 |
GP0303–0759 | 0.16488 | 7.86e | – | 15 000 |
GP1244+0216 | 0.23942 | 8.17e | – | 15 000 |
GP1054+5238 | 0.25264 | 8.10e | – | 15 000 |
GP0911+1831 | 0.26223 | 8.00e | – | 15 000 |
SGAS J1226 | 2.92525 | – | – | 4000 |
SGAS J1527 | 2.76228 | <8.5i | – | 2700 |
Cosmic Eye | 3.07483 | 8.60f | – | 2500 |
Notes. Column 1: Galaxy name; Col. 2: redshift; Col. 3: metallicities derived from optical emission lines; Col. 4: Lyman continuum escape fraction; and Col. 5: spectral resolution of the observations. Dashes indicate that the quantities have not been measured.
Reference.(a)Pettini & Pagel (2004); (b) Izotov et al. (2016b); (c) Izotov et al. (2016a); (d) Leitherer et al. (2016); (e) Izotov et al. (2011); (f) Stark et al. (2008); (g) Borthakur et al. (2014); (h)Chisholm et al. (2017a); (i)Wuyts et al. (2012).
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