Table 1.
General properties of the sample galaxies.
| Name | RA | Dec | Type | Redshift | Ngal | MBH | LBol | λEdd | |
|---|---|---|---|---|---|---|---|---|---|
| (J2000) | (J2000) | (1020 cm−2) | M⊙ | (log) | (log) | ||||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | |
| NGC 3998 | 179.484 | 55.454 | Sy1.9 | 0.003 | 20.09 | 8.93L | 42.29 | −4.74 | |
| NGC 3718 | 173.145 | 53.068 | Sy1.9 | 0.003 | 20.03 | 8.14 | 41.74 | −4.49 | |
| NGC 4258* | 184.740 | 47.304 | Sy1.9 | 0.001 | 20.08 | 7.56L | 41.39 | −4.28 | |
| NGC 5033 | 198.364 | 36.593 | Sy1.9 | 0.002 | 20.00 | 7.68 | 41.78 | −4.00 | |
| ESO 253-G003* | 81.325 | −46.00 | Sy2 | 0.042 | 20.62 | 9.84+ | 43.89 | −3.95 | |
| NGC 1052 | 40.270 | −8.256 | Sy2 | 0.005 | 20.49 | 8.67 | 42.83 | −3.94 | |
| NGC 2655 | 133.907 | 78.223 | Sy2 | 0.004 | 20.32 | 8.20 | 42.43 | −3.87 | |
| NGC 3147* | 154.223 | 73.400 | Sy2 | 0.009 | 20.54 | 8.81 | 43.10 | −3.81 | |
| NGC 2110* | 88.047 | −7.456 | Sy2 | 0.007 | 21.27 | 9.38 | 43.81 | −3.67 | |
| LEDA 96373* | 111.610 | −35.906 | Sy2 | 0.029 | 21.47 | 9.21 | 43.80 | −3.51 | |
| NGC 2992 | 146.425 | −14.326 | Sy1.9 | 0.007 | 20.72 | 8.33 | 43.13 | −3.30 | |
| M 51 | 202.484 | 47.230 | Sy2 | 0.001 | 20.19 | 6.59 | 41.40 | −3.29 | |
| NGC 2273* | 102.536 | 60.845 | Sy2 | 0.006 | 20.84 | 7.99 | 42.84 | −3.25 | |
| HE 1136-2304 | 174.713 | −23.360 | Sy1.9 | 0.027 | 20.63 | 9.39 | 44.28 | −3.21 | |
| IGRJ 11366-6002 | 174.175 | −60.052 | Sy1 | 0.014 | 21.81 | 8.56 | 43.51 | −3.15 | |
| IC 4518A | 224.421 | −43.132 | Sy2 | 0.016 | 20.96 | 8.79 | 43.83 | −3.06 | |
| NGC 7674* | 351.986 | 8.779 | Sy2 | 0.028 | 20.70 | 9.18 | 44.28 | −3.0 |
Notes. Column 1 Name, (Cols. 2 and 3) right ascension and declination in Equatorial (J2000.0) from Swift BAT 105-month hard X-ray survey (Oh et al. 2018), (Cols. 4, 5, 7, 8 and 9) optical classification from BASS/DR2, redshift, Black hole mass using the velocity dispersion method, bolometric luminosity and accretion rate λEdd = LBol/LEdd from BASS/DR2 survey (L identify masses taken from literature by the BASS/DR2 survey and the symbol + means from MgII). Column 6 represents the galactic absorption (Dickey & Lockman 1990). Objects marked with * are the galaxies with non-simultaneous observations with XMM-Newton and NuSTAR.
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