Table 2.
Current bolometric luminosity estimators.
| Source | L[OIII] | Lnearest | LFIR | LX | Ref. |
|---|---|---|---|---|---|
| (1) | (2) | (3) | (4) | (5) | (6) |
| SDSS1510+07 | 1.5 × 1043 | 2.1 × 1044 | 4 × 1044 | 1.6 − 2.4 × 1043 | Keel et al. (2012) |
| UGC 7342 | 1.2 × 1043 | 4.7 × 1045 | 1.1 × 1044 | Keel et al. (2012) | |
| SDSS1524+08 | 1.7 × 1044 | 1.3 × 1044 | 1.6 × 1044 | 6.12 − 11.5 × 1041 | Keel et al. (2012) |
| NGC 5972 | 8.3 × 1043 | 7.2 × 1044 | 5.5 × 1043 | 2.3 − 9.8 × 1043 | Keel et al. (2012), Zhao et al. (2021), Harvey et al. (2023) |
| The Teacup | 1.6 × 1045 | 2.2 × 1045 | 2.3 × 1043 | 8 − 140 × 1044 | Lansbury et al. (2018), Harrison et al. (2014), Keel et al. (2017) |
Notes. Columns: (1) Target name; (2) bolometric luminosity derived from [OIII] luminosity in the nucleus; (3) bolometric luminosity derived from the CLOUDY simulations in the nearest aperture to the nucleus; (4) FIR luminosity; (5) bolometric luminosity derived from X-ray (2–10 keV); (6) references. All luminosity values are in erg/s. Columns (2) and (3) are calculated in this work, as well as (5) for SDSS1510+07 and SDSS1524+08.
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