Table 3.
MCP reported parameters of the sample galaxies.
| Source | Position | Mass | Distance | M/D | Recession velocity | Inclination angle | |
|---|---|---|---|---|---|---|---|
| RA (h:m:s) | |||||||
| Dec (° : ′ : ″) | (107 M⊙) | (Mpc) | (105 M⊙)/Mpc | (km/s) | (°)(d) | ||
| NGC 1194 (e) | 03:03:49.10864 | 6.5 ± 0.3 | 55.4 ± 3.9 ( * ) | 11.733 | 4051 ± 15 | 85 (a) | |
| –01:06:13.4743 | |||||||
| NGC 5495 (f) | 14:12:23.35 | 1.1 ± 0.2 | 95.7 ± 5.3 | 1.149 | 6839.6 ± 67.0 | 95 ± 1 (b) | |
| –27:06 29.20 | |||||||
| Mrk 1029 (f) | 02:17:03.566 | 0.19 ± 0.05 | 120.8 ± 6.6 | 0.158 | 9129.9 ± 26.0 | 79 ± 2 (b) | |
| 05:17:31.43 | |||||||
| NGC 1320 (f) | 03:24:48.70 | 0.55 ± 0.25 | 34.2 ± 1.9 | 1.608 | 2829.2 ± 11.4 | 90 (c) | |
| –03:02:32.30 | |||||||
Notes. Column 1: Name of the source. Column 2: Source position (J2000). Column 3: Fitted mass of the SMBHs. Column 4: Estimated distance to the sources. Column 5: Computed M/D ratio from Columns 3 and 4. Column 6: Fitted recession velocities. Column 7: Reported inclination angle θ0 for NGC 1194, NGC 5495, and Mrk 1029 and fixed inclination angle for NGC 1320.
Label (a) represents values reported without uncertainty.
Label (b) refers to the inclination angle fixed through observations of systemic masers in Gao et al. (2016).
Label (c) refers to the fixed inclination angle due to the absence of systemic maser features in Gao et al. (2016).
Label (d) refers to the inclination angle fixed through observations of systemic masers in Zhao et al. (2018).
Label ( * ) indicates the distance to NGC 1194 estimated in Kamali et al. (2017).
Label (e) corresponds to the reference: Kuo et al. (2011).
Label (f) corresponds to the reference: Gao et al. (2016).
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