Table A.1.
Summary of the emission line and WISE colour fluxes used in this work and taken from the GAMA DR3 (Baldry et al. 2018).
| Model | HATLAS090750 | HATLAS114625 | HATLAS121446 |
|---|---|---|---|
| fHβ (×10−17 erg s−1 cm−2) | 552 ± 16 | 76 ± 23 | 29 ± 11 |
| f[O III] (×10−17 erg s−1 cm−2) | 402 ± 14 | 196 ± 34 | 11 ± 8 |
| fHα (×10−17 erg s−1 cm−2) | 2680 ± 33 | 307 ± 18 | 588 ± 25 |
| f[N II] (×10−17 erg s−1 cm−2) | 1016 ± 17 | 444 ± 17 | 286 ± 17 |
| W1 (mJy) | 1.15 ± 0.03 | 1.57 ± 0.03 | 0.59 ± 0.02 |
| W2 (mJy) | 1.04 ± 0.03 | 2.40 ± 0.05 | 0.66 ± 0.02 |
| W3 (mJy) | 16.89 ± 0.41 | 11.99 ± 0.34 | 8.65 ± 0.35 |
Notes. W1, W2, and W3 correspond to the “profile-fit photometry” WISE filter fluxes measured at 3.4, 4.6, and 12 μm (Cluver et al. 2014). The uncertainties indicate 1-σ errors. Our three galaxies are catalogued as unresolved by WISE.
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