Table 1.
Properties of the five QSO2s.
| SDSS ID | z | Scale | log L[O III] | log Lbol | log L1.4 GHz | log M* | SFR | Galaxy |
|---|---|---|---|---|---|---|---|---|
| SDSS | [kpc arcsec−1] | [erg s−1] | [erg s−1] | [W Hz−1] | [M⊙] | [M⊙ yr−1] | morphology | |
| J101043.36+061201.4 | 0.0977 | 1.807 | 42.88 | 45.55 | 24.37 | 10.99±0.20 | 30 | Interacting ETG |
| J110012.39+084616.3 | 0.1004 | 1.851 | 43.18 | 45.85 | 24.18 | 11.02±0.22 | 34 | Barred spiral |
| J135646.10+102609.0 | 0.1232 | 2.213 | 42.87 | 45.54 | 24.36 | 11.27±0.19 | 69 | Merging ETG |
| J143029.88+133912.0 | 0.0851 | 1.597 | 43.16 | 45.83 | 23.67 | 11.15±0.11 | 12 | Post-merger ETG |
| J150904.22+043441.8 | 0.1115 | 2.028 | 43.37 | 46.04 | 23.81 | 10.94±0.31 | 34 | Barred spiral |
Notes. The bolometric luminosities were calculated by applying the correction factor of 474 from Lamastra et al. (2009) to the extinction-corrected [O III] luminosities from Kong & Ho (2018). The 1.4 GHz luminosities, stellar masses, SFRs, and galaxy morphologies are from Ramos Almeida et al. (2022).
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