Table 3.
Black hole masses retrieved from literature and spectroscopic data used to estimate MBH through MgII-based virial relation.
| No. (a) | Object ID | FWHM(MgII) | λLλ(3000 Å) | MBH(b) | References |
|---|---|---|---|---|---|
| (km s−1) | (1046 erg s−1) | (M⊙) | |||
| 2 | VHS J2101−5943 | – | – | 3.2 ± 0.7 × 1010 | Ban2015 |
| 6 | SDSS J1328−0224 | 3815 ± 954 | 1.9 ± 0.4 | 8 ± 4 × 108 | Tra2011 |
| 7 | SDSS J0923+0247 | 2636 ± 264 | 1.4 ± 0.3 | 3.3 ± 1.0 × 108 | Tra2011 |
| 9 | SDSS J0129−0035 | – | – |
 |
Wan2013 |
| 10 | SDSS J1044−0125 | – | – | 5.6 ± 0.5 × 109 | She2019 |
| 11 | SDSS J1306+0356 | 3158 ± 145 | 2.45 ± 0.06 | 6.3 ± 1.5 × 108 | DeR2011 |
| 12 | SDSS J2310+1855 | 4497 ± 352 | 6.027 ± 0.018 | 2.0 ± 0.6 × 109 | She2019 |
| 14 | SDSS J2054−0005 | – | – |
 |
Wan2013 |
| 19 | ULAS J1319+0950 | 3675 ± 17 | 3.8 ± 1.0 | 1.1 ± 0.2 × 109 | Sha2017 |
| 26 | PSO J167−13 | 2350 ± 470 | 1.5 ± 0.7 | 2.7 ± 1.4 × 108 | Ven2015 |
| 28 | VIKING J0305−3150 | 3189 ± 85 | 1.66 ± 0.02 | 5.2 ± 1.2 × 108 | DeR2014 |
Notes.
Source identification numbers in agreement with those listed in the first column of Table 1.
Black hole mass estimated using SE virial relation in Eq. (5) when possible, otherwise, the value provided here is the one available in literature (see references for full details). The uncertainties we report do not include the systematic uncertainties intrinsic to the MBH estimators.
References. Ban2015 – Banerji et al. (2015); DeR2011, DeR2014 – De Rosa et al. (2011, 2014); Sha2017 – Shao et al. (2017); She2019 – Shen et al. (2019); Tra2011 – Trakhtenbrot et al. (2011); Ven2015 – Venemans et al. (2015); Wan2013 – Wang et al. (2013).
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