Table 3.
Emission line fluxes for the apertures and derived quantities ionised gas mass and star formation rate.
| Aperture | [Fe II] | Paα | Brδ | He I | Brγ | H II mass | SFR |
|---|---|---|---|---|---|---|---|
| λ1.644 μm | λ1.876 μm | λ1.945 μm | λ2.059 μm | λ2.166 μm | [104 M⊙] | [10−3 M⊙ yr−1] | |
| N (*) | 18 ± 4 | – | – | – | 8 ± 2 | 5.2 | 13 |
| 1 | 16.0 ± 1.2 | 90.9 ± 1.8 | 3.9 ± 1.0 | 2.5 ± 0.5 | 10.3 ± 0.6 | 6.6 | 17 |
| 2 | 9.1 ± 1.1 | 75.4 ± 1.9 | 4.2 ± 1.0 | 3.6 ± 0.5 | 10.1 ± 0.6 | 6.5 | 17 |
| 3 | 16.6 ± 1.4 | 27.2 ± 2.3 | 13.1 ± 1.3 | 4.6 ± 0.9 | 17.1 ± 0.6 | 11.0 | 29 |
| 4 | 14.0 ± 1.3 | 37.8 ± 2.0 | 3.8 ± 1.3 | 4.2 ± 1.1 | 9.5 ± 0.7 | 6.1 | 16 |
| 5 | 30.5 ± 1.5 | 160.6 ± 2.9 | 12.0 ± 1.1 | 8.2 ± 0.9 | 19.6 ± 0.9 | 12.6 | 33 |
| 6 | 38.6 ± 1.7 | 82.0 ± 2.7 | 13.7 ± 1.3 | 11.3 ± 0.6 | 27.9 ± 0.9 | 17.9 | 47 |
| 7 | 44.8 ± 1.7 | 43.5 ± 2.6 | 21.8 ± 1.2 | 10.5 ± 0.7 | 31.0 ± 1.1 | 19.9 | 52 |
| 8 | 10.2 ± 5.0 (+) | 39.0 ± 5.1 | 0.8 ± 0.0 | 6.2 ± 1.3 | 7.1 ± 1.5 | 4.6 | 12 |
| 9 | 16.7 ± 4.7 | 18.0 ± 4.1 | 2.5 ± 2.6 | 3.6 ± 1.0 | 7.3 ± 1.2 | 4.7 | 12 |
| 10 | 10.2 ± 5.0 (+) | – | – | – | 7.1 ± 1.5 | 3.3 | 9 |
| 11 | – | – | – | – | 7.4 ± 1.2 | 2.2 | 6 |
Notes. The flux units are 10−19 W m−2. (*)For the nuclear aperture we reported the extinction value in Table 1, however, the flux values for this aperture are not corrected for extinction because of AGN contamination of H − K-colour. (+)The emission line fit values have uncertainties higher than 30%. However, the emission line fit reveals a line, therefore we report the flux in the table.
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