Table 1.
Properties of the sample galaxies.
| Galaxy | Morph. | AGN | d | i | Scale | Lbol | M⚫ | λEdd |
|---|---|---|---|---|---|---|---|---|
| ID | type | type | (Mpc) | (°) | (pc arcsec−1) | (erg s−1) | (M⊙) | |
| Mrk 1044 | SAB0/a | NLSy1 | 69.5 | 36 | 332 | 1.42 ± 0.14 × 1044 | 2.8 ± 0.8 × 106 | 0.34 ± 0.10 |
| NGC 3783 | (R′)SB(r)ab | Sy 1.5 | 41.0 | 24 | 197 | 1.8 × 1044 | 2.34 ± 0.43 × 107 | 0.052 ± 0.010 |
| NGC 4593 | (R)SB(rs)b | Sy 1 | 35.4 | 34 | 170 | 5 × 1043 | 9.8 ± 2.1 × 106 | 0.035 ± 0.007 |
| NGC 7130 | Sa pec | Sy 1.9 | 68.7 | 32 | 328 | 2.5 × 1044 | – | – |
Notes. The references for the properties of the galaxies are given within the subsections corresponding to each galaxy in Sect. 2. Here d stands for the comoving distance, i for the inclination, Lbol for the bolometric luminosity, M⚫ for the SMBH mass, and λEdd for the Eddington ratio. The values of Lbol and M⚫ are not corrected for the different distance estimates. The error in λEdd is based on the propagation of the error in M⚫. For NGC 7130 we do not present an Eddington ratio due to the lack of an accurate SMBH mass measurement.
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