Table 1.
Main properties of the BCS40 sample.
| Name | RA | Dec | DL | Spatial | Sy | log (NH) | log ( ) |
log (MBH/M⊙) | log (λEdd) |
|---|---|---|---|---|---|---|---|---|---|
| (J2000) | (J2000) | (Mpc) | scale | type | (cm−2) | (erg s−1) | |||
| (pc/arcsec) | |||||||||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) |
| NGC 1365 | 03h33m36.4s | −36d08m25s | 21.5 | 103 | 1.8 | 22.21 | 42.32 | 7.92 (a) | −2.44 |
| NGC 2110 | 05h52m11.4s | −07d27m22s | 32.4 | 155 | 2.0 | 22.94 | 42.69 | 9.25 (b) | −3.40 |
| ESO 005-G004 | 06h05m41.6s | −86d37m55s | 24.1 | 116 | 2.0 | 24.34 | 42.78 | 6.98 (c) | −1.04 |
| NGC 2992 | 09h45m42.0s | −14d19m35s | 34.4 | 164 | 1.9 | 21.72 | 42.00 | 5.42 (b) | −0.26 |
| MCG-05-23-016 | 09h47m40.1s | −30h56m55s | 35.8 | 171 | 2.0 | 22.18 | 43.20 | 7.98 (a) | −1.62 |
| NGC 3081 | 09h59m29.5s | −22d49m35s | 34.5 | 164 | 2.0 | 23.91 | 42.72 | 8.41 (b) | −2.53 |
| NGC 3227 | 10h23m30.6s | +19d51m54s | 20.4 | 98 | 1.5 | 20.95 | 42.10 | 6.62 (b) | −1.36 |
| NGC 3783 | 11h39m01.7s | −37d44m19s | 36.4 | 173 | 1.2 | 20.49 | 43.43 | 7.14 (a) | −0.55 |
| UGC 6728 | 11h45m16.0s | +79d40m53s | 32.1 | 153 | 1.2 | 20.00 | 41.80 | 5.32 (b) | −0.36 |
| NGC 4051 | 12h03m09.6s | +44d31m53s | 12.9 | 62 | 1.2 | 20.00 | 41.33 | 5.60 (b) | −1.11 |
| NGC 4138 | 12h09m29.8s | +43d41m07s | 17.7 | 85 | 1.9 | 22.89 | 41.23 | 7.30 (b) | −2.91 |
| NGC 4151 | 12h10m32.6s | +39d24m21s | 20.0 | 96 | 1.5 | 22.71 | 42.31 | 7.43 (a) | −1.96 |
| NGC 4388 (*) | 12h25m46.7s | +12d39m44s | 17.0 | 82 | 2.0 | 23.52 | 43.05 | 6.99 (b) | −0.78 |
| NGC 4395 | 12h25m48.8s | +33d32m49s | 3.84 | 19 | 1.8 | 21.04 | 40.50 | 4.88 (a) | −1.22 |
| NGC 4945 | 13h05m27.5s | −49d28m06s | 4.36 | 21 | 2.0 | 24.80 | 42.69 | 7.78 (a) | −1.93 |
| NGC 5128/CenA | 13h25m27.6s | −43d01m09s | 4.28 | 21 | 2.0 | 23.02 | 42.39 | 7.94 (a) | −2.39 |
| MCG-06-30-015 | 13h35m53.7s | −34d17m44s | 26.8 | 128 | 1.2 | 20.85 | 42.74 | 7.42 (a) | −1.52 |
| NGC 5506 | 14h13m14.9s | −03d12m27s | 30.1 | 144 | 1.9 | 22.44 | 42.99 | 8.29 (a) | −2.14 |
| NGC 6300 | 17h16m59.5s | −62d49m14s | 14.0 | 68 | 2.0 | 23.31 | 41.84 | 7.01 (a) | −2.01 |
| NGC 6814 | 19h42n40.6s | −10d19m25s | 25.8 | 123 | 1.5 | 20.97 | 42.31 | 6.46 (b) | −0.99 |
| NGC 7172 | 22h02m01.9s | −31d52m11s | 37.9 | 180 | 2.0 | 22.91 | 42.76 | 8.45 (b) | −2.53 |
| NGC 7213 | 22h09m16.3s | −47d10m00s | 25.1 | 120 | 1.5 | 20.00 | 41.95 | 7.37 (c) | −2.26 |
| NGC 7314 | 22h35m46.2s | −26d03m02s | 20.9 | 100 | 1.9 | 21.60 | 42.33 | 7.24 (b) | −1.75 |
| NGC 7582 | 23h18m23.5s | −42d22m14s | 22.1 | 106 | 2.0 | 24.33 | 42.86 | 7.52 (a) | −1.50 |
Notes. Right ascension (RA), declination (Dec) and Seyfert type. (*)This galaxy is part of the Virgo Cluster (Binggeli et al. 1985). We assumed a cosmology with H0 = 70 km s−1 Mpc−1, Ωm = 0.3, and ΩΛ = 0.7, and a velocity-field corrected using the Mould et al. (2000) model, which includes the influence of the Virgo cluster, the Great Attractor, and the Shapley supercluster. The X-ray hydrogen column density and intrinsic 2–10 keV X-ray luminosity were taken from Ricci et al. (2017b). References for the BH masses: (a) GB19; (b) Koss et al. (2017); (c) Vasudevan et al. (2010). We note that the Eddington ratio is derived following the methodology as in Ricci et al. (2017a).
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