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Table 5

Si II covering fractions.

Galaxy name Si II 1190 Å Si II 1260 Å Mean
(1) (2) (3) (4)
J0921+4509 0.66 ± 0.32 0.59 ± 0.15 0.60 ± 0.14
J1503+3644 0.38 ± 0.35 0.56 ± 0.45 0.45 ± 0.28
J0925+1409 0.40 ± 0.23 0.43 ± 0.34 0.41 ± 0.19
J1152+3400 0.27 ± 0.26 0.23 ± 0.55 0.27 ± 0.24
J1333+6246 0.29 ± 0.26 0.56 ± 0.35 0.39 ± 0.21
J1442–0209 0.46 ± 0.23 0.48 ± 0.34 0.47 ± 0.19
Tol1247–232 0.26 ± 0.01 0.26 ± 0.01
Tol0440–381 0.37 ± 0.04 0.37 ± 0.04
Mrk54 0.32 ± 0.01 0.32 ± 0.01
J0926+4427 0.37 ± 0.19 0.36 ± 0.06 0.36 ± 0.06
J1429+0643 0.73 ± 0.26 0.78 ± 0.11 0.77 ± 0.10
GP0303–0759 0.54 ± 0.29 0.47 ± 0.12 0.48 ± 0.11
GP1244+0216 0.49 ± 0.39 0.51 ± 0.18 0.50 ± 0.16
GP1054+5238 0.41 ± 0.34 0.49 ± 0.22 0.46 ± 0.19
GP0911+1831 0.39 ± 0.36 0.45 ± 0.33 0.43 ± 0.24
SGAS J1226 0.97 ± 0.06 0.91 ± 0.04 0.93 ± 0.03
SGAS J1527 0.83 ± 0.16 0.79 ± 0.10 0.80 ± 0.08
Cosmic Eye 0.98 ± 0.06 0.94 ± 0.03 0.95 ± 0.02

Notes. Column 1: Galaxy name; Col. 2: Cf(Si II) derived from the Si II 1190 Å doublet using Eq. (11); Col. 3: Cf(Si II) derived fromthe Si II 1260 Å absorption line; Col. 4: weighted mean between Cols. 2 and 3. We do not observe the Si II 1190 Å doublet for Tol1247–232, Tol0440–381, and Mrk54 because these lines fall in the COS detector gap.

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