Partial alignment between jets and megamasers: Coherent versus selective accretion

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Table 1.

Main properties of the sample.

Name	Redshift	log(M_gal/M_⊙)	log(M_BH/M_⊙)
NGC 3079	0.004	10.29	6.38 ± 0.1 ^(a)
NGC 2273	0.006	10.59	6.88 ± 0.05 ^(b)
NGC 1068	0.004	10.84	7.24 ± 0.003 ^(c)
NGC 2960	0.017	10.76	7.05 ± 0.05 ^(b)
UGC 3789	0.011	10.42	7.05 ± 0.05 ^(b)
NGC 1194	0.014	10.81	7.82 ± 0.05 ^(b)
NGC 3393	0.013	10.74	7.49 ± 0.12 ^(b)
NGC 4388	0.008	10.8	6.93 ± 0.05 ^(b)
Circinus	0.001	10.88	6.06 ± 0.1 ^(d)
NGC 4258	0.002	10.43	7.6 ± 0.01 ^(e)

Notes. All redshifts are obtained from NASA/NED. The stellar masses of the hosts are obtained from colors (based on NASA/NED absolute magnitudes), following Zibetti et al. (2009). Typical uncertainties on the stellar masses are ∼10%. The MBH masses are from:

^(a)

Yamauchi et al. (2004),

^(b)

Greene et al. (2010),

^(c)

Gallimore & Impellizzeri (2023),

^(d)

Greenhill et al. (2003),

^(e)

Humphreys et al. (2013).

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