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 | 3.1 | 0.6 | 6.0 | 0.9 | 4.0 | 0.5 | 1.3 | 0.6 | 2.8 | 0.6 | 3.6 | 0.7 | 3.2 | 1.1 |
1036 | 3.0 | 1.1 | 12.4 | 0.8 | 8.5 | 1.0 | 2.1 | 0.7 | 4.8 | 0.7 | 4.6 | 0.6 | 2.5 | 0.8 |
1045 | 3.6 | 0.9 | 11.5 | 1.2 | 6.3 | 1.1 | 3.2 | 0.8 | 4.6 | 0.8 | 4.1 | 0.7 | 3.8 | 0.8 |
1079 | 8.2 | 2.0 | 21.3 | 1.8 | 14.4 | 1.5 | 3.6 | 1.1 | 7.2 | 1.4 | 7.3 | 1.9 | 3.0 | 1.4 |
1273 | 10.3 | −99.0 | 7.2 | −99.0 | 12.4 | −99.0 | 10.2 | −99.0 | 10.1 | −99.0 | 14.5 | −99.0 | 7.0 | −99.0 |
3621 | 4.8 | 0.8 | 7.1 | 0.8 | 3.0 | 0.8 | 2.1 | 0.5 | 3.8 | 0.5 | 2.9 | 0.5 | 4.1 | 0.7 |
87 | 3.2 | 0.4 | 5.7 | 0.5 | 5.0 | 0.5 | 1.5 | 0.5 | 4.3 | 0.5 | 4.5 | 0.7 | 2.2 | 0.7 |
109 | 10.7 | 2.2 | – | – | – | – | 9.7 | 1.8 | 37.2 | 4.3 | – | – | – | – |
144 | 17.9 | 2.4 | 28.9 | 3.1 | 20.2 | 3.8 | 8.8 | 1.4 | 16.9 | 1.9 | 7.7 | 1.9 | 3.0 | 1.8 |
97 | 24.7 | −99.0 | – | – | – | – | 5.1 | −99.0 | 1.3 | −99.0 | – | – | – | – |
39 | 26.9 | 3.5 | 18.6 | −99.0 | 12.0 | −99.0 | 8.5 | 2.4 | 6.3 | 2.0 | 39.4 | −99.0 | 23.3 | −99.0 |
84 | 50.3 | −99.0 | 10.4 | −99.0 | 0.3 | −99.0 | 1.7 | −99.0 | 6.9 | −99.0 | 6.6 | −99.0 | 12.0 | −99.0 |
161 | 9.1 | 2.6 | 0.7 | 0.6 | 1.5 | 0.7 | 0.2 | 0.7 | 0.2 | 0.4 | 0.0 | 0.4 | 0.4 | 0.6 |
Notes. All EWs are in Å. EW errors were obtained from bootstrap resampling of the spectrum 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 was 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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