Table 3.
EWs of the MUSE He II λ1640 sample used in this analysis.
| ID | He II λ1640 |
[C III]1907 |
C III]1909 |
O III]1661 |
O III]1666 |
Si III]1883 |
Si III]1892 |
|||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| EW | ΔEW | EW | ΔEW | EW | ΔEW | EW | ΔEW | EW | ΔEW | EW | ΔEW | EW | ΔEW | |
| 1024 | 18.9 | 3.5 | 18.5 | 3.1 | 20.5 | 3.5 | 23.2 | 3.6 | 21.7 | 3.3 | 20.9 | 3.2 | 21.3 | 3.0 |
| 1036 | 12.9 | 2.9 | 4.4 | 1.0 | 8.3 | 1.4 | 14.7 | 1.1 | 12.0 | 1.1 | 12.2 | 0.9 | 14.3 | 1.2 |
| 1045 | 12.6 | 2.2 | 6.6 | 1.2 | 11.8 | 1.7 | 14.9 | 1.3 | 13.5 | 1.4 | 14.0 | 1.3 | 14.3 | 1.7 |
| 1079 | 35.6 | 11.5 | 16.6 | 0.7 | 15.8 | 0.7 | 17.1 | 0.6 | 17.5 | 0.7 | 17.3 | 0.6 | 16.9 | 0.7 |
| 1273 | 13.7 | 3.7 | 6.5 | 2.0 | 0.4 | 1.0 | 11.2 | 1.6 | 7.6 | 1.1 | 7.5 | 1.6 | 11.8 | 1.7 |
| 3621 | 6.8 | – | 9.3 | – | 15.3 | – | 11.5 | – | 11.4 | – | 16.6 | – | 10.2 | – |
| 87 | 11.4 | 2.1 | 5.5 | 0.7 | 9.6 | 0.7 | 10.5 | 0.7 | 8.8 | 0.6 | 9.7 | 0.6 | 8.5 | 0.9 |
| 109 | 11.0 | 1.0 | 8.7 | 0.7 | 9.4 | 0.7 | 12.9 | 0.8 | 10.1 | 0.6 | 9.9 | 1.0 | 12.2 | 0.9 |
| 144 | 5.2 | 1.5 | – | – | – | – | 2.9 | 1.9 | 24.6 | 3.0 | – | – | – | – |
| 97 | 5.5 | 2.3 | 14.0 | 2.7 | 5.3 | 4.4 | 6.1 | 1.5 | 2.0 | 2.0 | 7.2 | 2.2 | 11.9 | 2.0 |
| 39 | 3.6 | – | – | – | – | – | 4.7 | – | 9.6 | – | – | – | – | – |
| 84 | 8.5 | 2.9 | 8.9 | – | 3.4 | – | 4.1 | 2.2 | 6.3 | 1.6 | 32.0 | – | 14.2 | – |
| 161 | 28.3 | – | 11.7 | – | 1.5 | – | 5.7 | – | 2.7 | – | 6.8 | – | 12.6 | – |
Notes. All EWs are in Å. EW errors are obtained from bootstrap resampling of the spectrum (see Sect. 2.3) and account for the uncertainty in continuum fitting. If a line is not covered by the spectral range of MUSE, the EW is shown by a long dash. If a line is covered but the continuum level around the considered line is below the error level, the ΔEW is shown by a long dash. In these cases, the EW is computed assuming that the continuum level equals the noise level, and the EW presented should be considered as a lower limit.
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