Table 1.
Rest-frame EWs of bright optical emission lines for the ASK templates considered EELGs.
| ASK class | EW(Hβ) | EW([OIII]λ5007) | EW(Hα) | log(O/H) + 12 ( * ) |
|---|---|---|---|---|
| (Å) | (Å) | (Å) | ||
| 15 | 169.6 | 1097.9 | 918.3 | 8.00 (a) |
| 17 | 144.9 | 874.3 | 782.3 | 8.09 |
| 20 | 92.3 | 496.2 | 484.9 | 8.23 |
| 21 | 85.9 | 460.1 | 457.5 | 8.20 |
| 25 | 63.9 | 298.1 | 334.4 | 8.32 |
| 26 | 45.1 | 172.8 | 232.0 | 8.42 |
| 27 | 57.4 | 234.1 | 302.4 | 8.37 |
Notes. The obtained values are comparable with the measurements reported in Sánchez Almeida et al. (2010). ( * )Based on O32 calibration from Bian et al. (2018).
[OII]λλ3727,3729 outside the observed spectral range. Metallicity based on the code HII-CHI-mistry (Pérez-Montero et al. 2021).
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