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Table 2
Frequency of the different types of nuclear spectra in the whole HRS sample (left) and among the 254 LTGs (right), including galaxies a posteriori classified as passive or post-starburst.
| heightBPT ([NII]/Hα) 255∕322 | AGN 34 (13%) | BPT ([NII]/Hα) 206∕254 | AGN 26 (13%) |
|---|---|---|---|
| TRAN 31 (12%) | TRAN 27 (13%) | ||
| HII 152 (60%) | HII 149 (72%) | ||
| PAS 36 (14%) | PAS 2 (1%) | ||
| PSB 2 (1%) | PSB 2 (1%) | ||
| BPT ([SII]/Hα) 255∕322 | SEY 23 (9%) | BPT ([SII]/Hα) 206∕254 | SEY 20 (10%) |
| LIN 30 (12%) | LIN 24 (11%) | ||
| HII 164 (64%) | HII 158 (77%) | ||
| PAS 36 (14%) | PAS 2 (1%) | ||
| PSB 2 (1%) | PSB 2 (1%) | ||
| WHAN 322∕322 | sAGN 24 (7%) | WHAN 254∕254 | sAGN 21 (8%) |
| wAGN 63 (20%) | wAGN 47 (19%) | ||
| HII 171 (53%) | HII 168 (67%) | ||
| RET 28 (9%) | RET 14 (6%) | ||
| PAS 34 (11%) | PAS 2 (0.5%) | ||
| PSB 2 (1%) | PSB 2 (0.5%) | ||
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