Table 1.
Sample of galaxies sorted by decreasing Eddington rate λEdd.
| Name | Type | Host | D | RefD | log(MBH) | RefBH | log(LX) | RefX | log(Lbol) | log( ) |
 |
FWHM | 1″ | AV |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| (Mpc) | (M⊙) | (erg s−1) | (erg s−1) | (erg s−1) | (pc) | (pc) | (mag) | |||||||
| NGC 1386 | Sy2 | SB(s)a | 15.3 | JEN03 | 7.72 | HLED | 42.15 | MAS16 | 42.34 | 42.65 | −3.17 | 6.7 | 74.2 | 0.034 |
| NGC 1097 | LINb | SB(r′l)b | 14.2 | TUL09 | 7.17 | DAV07 | 40.63 | NEM06 | 41.79 | 41.89 | −3.38 | 8.9 | 68.8 | 0.073 |
| NGC 1052 | LINb | E4 | 18.0 | JEN03 | 8.56 | HLED | 41.33 | GON09 | 42.84 | 42.88 | −3.78 | 10.5 | 87.3 | 0.073 |
| NGC 4579 (M58) | LINb | SAB(rs)b | 16.7 | TUL13 | 8.13 | HLED | 41.39 | GON09 | 42.41 | 42.35 | −3.88 | 6.3 | 81.0 | 0.112 |
| NGC 3169 | LIN | SA(s)a | 24.7 | MAN09 | 8.38 | HO09 | 41.61 | TER03 | 42.10 | 42.50 | −3.98 | 10.9 | 119.7 | 0.085 |
| NGC 4261 (3C 270) | LINb | E2-3 | 32.4 | TUL13 | 8.72 | FER96 | 41.22 | GON09 | 42.24 | 42.51 | −4.31 | 12.3 | 157.1 | 0.049 |
| M87 (3C 274) | LINb | cD | 16.7 | BLA09 | 9.79 | GEB11 | 40.49 | PRI16 | 42.45 | 42.32 | −5.57 | 9.2 | 81.0 | 0.063 |
| NGC 4594 (Sombrero) | LIN | SA(s)a | 9.08 | JEN03 | 8.82 | JAR11 | 40.00 | GON06 | 41.65 | 41.40 | −5.70 | 3.1 | 44.0 | 0.140 |
| NGC 404 | LIN | SA(s)0 | 3.05 | DAL09 | 5.65 | SET10 | 37.13 | PAR14 | < 40.37 | – | < − 3.38 | 1.2 | 14.8 | 0.160 |
Notes. The spatial resolution is estimated as the FWHM of the most compact object found in the FOV. In all cases, the Galactic extinction has been corrected using the reddening values from Schlafly & Finkbeiner (2011) and the extinction curve from Cardelli et al. (1989). LX is the luminosity in the 2–10 keV range, scaled to our adopted distance and corrected from absorption. Lbol is the bolometric luminosity extracted from the high-resolution continuum flux density distributions. 
is the integrated luminosity derived from the best-fit broken power law. In the case of NGC 4594, 
includes also a thermal component to account for the cold disc emission peaking at 1 μm.
References. For the redshift-independent distances. BLA09: Blakeslee et al. (2009); DAL09: Dalcanton et al. (2009); JEN03: Jensen et al. (2003); MAN09: Mandel et al. (2009); TUL09: Tully et al. (2009); TUL13: Tully et al. (2013). References for the BH mass estimates. FER96: Ferrarese et al. (1996); GEB11: Gebhardt et al. (2011); HLED, DAV07, HO09: based on the velocity dispersion given by HyperLEDA (Makarov et al. 2014), Davies et al. (2007), or by Ho et al. (2009), using the MBH–σ relation from Kormendy & Ho (2013); JAR11: Jardel et al. (2011); SET10: Seth et al. (2010). References for the X-ray luminosities. PAR14: Paragi et al. (2014); GON06: González-Martín et al. (2006); NEM06: Nemmen et al. (2006); MAS16: Masini et al. (2016); PRI16: Prieto et al. (2016); GON09: González-Martín et al. (2009); TER03: Terashima & Wilson (2003).
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