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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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