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Table 1.
Median line equivalent widths (in Å) for the whole working sample (all, 89 galaxies), strong leakers only (20 galaxies), and weak+nonleakers (69 galaxies).
| Ion + | Wλ (Å) | Wλ (Å) | Wλ (Å) |
|---|---|---|---|
| λrf (Å) | all (89) | strong leakers (20) | weak+nonleakers (69) |
| O I+Ly930 | 2.75 | 2.05 | 2.94 |
| O I+Ly938 | 1.71 | 1.41 | 1.80 |
| O I+Ly950 | 2.09 | 1.62 | 2.24 |
| O I+Ly973 | 2.78 | 1.58 | 3.15 |
| O I+N III+Si II989 | 0.77 | 0.60 | 0.83 |
| Si II1020 | 1.13 | 0.57 | 1.32 |
| O I+Ly1026 | 1.64 | 0.58 | 1.97 |
| Si II1190,1193 | 0.96 | 0.17 | 1.21 |
| Si II1260 | 0.96 | 0.56 | 1.08 |
| O I+Si II1302 | 1.08 | 0.64 | 1.21 |
| C II1334 | 0.79 | 0.52 | 0.88 |
Notes. Leakers have lower median equivalent widths than nonleaking galaxies in most cases.
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