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Table 3.
Emission lines fluxes and ratios, and BPT and WHAN classification computed through FADO with the integrated spectra (fluxes are in units of ×1016 erg/s/cm2).
| Galaxy | Hα | Hβ | log([N II]/Hα) | log([O III]/Hβ) | BPT | WHAN |
|---|---|---|---|---|---|---|
| VGS_31a | 1569 ± 2 | 466 ± 3 | −0.574 ± 0.001 | 0.116 ± 0.003 | SF | SF |
| VGS_31b | 2849 ± 3 | 804 ± 4 | −0.458 ± 0.001 | −0.132 ± 0.003 | SF | SF |
| VGS_31c | 286 ± 7 | 74 ± 6 | −0.953 ± 0.045 | 0.436 ± 0.036 | SF | SF |
| CAVITY52731 | 188 ± 4 | 27 ± 3 | −0.187 ± 0.019 | 0.661 ± 0.044 | Seyfert | wAGN |
| CAVITY52732 | 313 ± 2 | 85 ± 2 | −0.568 ± 0.006 | −0.114 ± 0.016 | SF | SF |
| CAVITY52733 | 202 ± 1 | 55 ± 1 | −0.452 ± 0.005 | −0.173 ± 0.017 | SF | SF |
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