Table 2
Sample properties.
| Galaxy | Distance | 33 GHz flux | rms | NVSS flux | FIRST flux | IR magnitude | Hard X-ray flux | log LH2O | Type of | |
| (Mpc) | (mJy) | (μJy/beam) | (mJy) | (mJy) | (10-11 erg s-1 cm-2) | (L⊙) | activity | |||
|
|
||||||||||
| ESO558-G009 | 112.2 ± 7.9 | 0.80 ± 0.04 | 18.6 | 12.8 ± 0.6 | ... | 8.793 | <0.34 | 2.9 | U | |
| IC 0485 | 122.0 ± 8.5 | ... | 18.9 | ... | 3.01 | 9.406 | 1.75  |
3.1 | U | |
| IC 2560 | 46.4 ± 3.3 | 2.00 ± 0.10 | 17.3 | 32.0 ± 1.7 | ... | 9.294 | 0.41 |
2.1 | Sy2 | |
| J0126-0417 | 76.2 ± 5.4 | 0.13 ± 0.01 | 9.9 | ... | ... | 8.930 | <0.34 | 2.1 | U | |
| J0350-0127 | 174.2 ± 12.2 | 0.14 ± 0.02 | 12.0 | ... | ... | 8.529 | 0.45 |
3.7 | U | |
| J0437+2456 | 68.1 ± 4.8 | ... | 17.7 | ... | ... | 9.024 | <0.41 | 2.3 | U | |
| J0437+6637 | 52.9 ± 3.7 | 0.11 ± 0.02 | 16.8 | 3.8 ± 0.6 | ... | 8.934 | 0.29 ± 0.14 | 1.4 | U | |
| J0836+3327 | 214.6 ± 15.0 | ... | 30.9 | ... | 1.95 | 9.145 ± 0.459 | <0.33 | 3.6 | Sy2 | |
| J1658+3923 | 146.8 ± 10.3 | 0.18 ± 0.04 | 13.4 | ... | 3.64 | 9.513 | <0.30 | 2.9 | Sy2 | |
| Mrk 0001 | 64.2 ± 4.5 | 3.96 ± 0.12 | 10.8 | 75.9 ± 2.3 | ... | 9.105 | <0.32 | 1.9 | Sy2 | |
| Mrk 0078 | 159.9 ± 11.2 | 1.75 ± 0.11 | 13.7 | 36.9 ± 1.2 | ... | 8.975 | 0.63 ± 0.18 | 1.6 | Sy2 | |
| Mrk 1029 | 126.0 ± 8.8 | 1.18 ± 0.14 | 17.7 | 11.9 ± 0.6 | 8.12 | 8.799 | <0.35 | 2.8 | U | |
| Mrk 1210 | 61.3 ± 4.3 | 9.58 ± 0.08 | 17.9 | 114.9 ± 3.5 | ... | 8.523 | 3.58 ± 0.20 | 2.0 | Sy2, Sy1 | |
| Mrk 1419 | 75.3 ± 5.3 | 0.36 ± 0.06 | 16.0 | 7.4 ± 0.5 | 5.13 | 8.790 | <0.34 | 2.7 | LINER | |
| NGC 0591 | 61.1 ± 4.3 | 1.52 ± 0.07 | 13.6 | 33.3 ± 1.1 | ... | 8.566 | 0.37 |
1.5 | Sy2 | |
| NGC 1194 | 55.4 ± 3.9 | 1.08 ± 0.04 | 13.0 | ... | 1.49 | 8.807 | 2.21 ± 0.18 | 2.8 | Sy 1.9 | |
| NGC 2273 | 26.8 ± 1.9 | 2.69 ± 0.29 | 26.3 | 63.4 ± 2.4 | ... | 9.734 ± 0.511 | 0.67 ± 0.16 | 0.9 | Sy2 | |
| NGC 2979 | 43.8 ± 3.1 | 0.36 ± 0.04 | 14.0 | 15.7 ± 1.0 | ... | 9.158 | <0.36 | 2.2 | Sy2 | |
| NGC 3393 | 58.6 ± 4.1 | 5.30 ± 0.36 | 18.5 | 81.5 ± 3.3 | ... | 8.846 | 1.56 ± 0.19 | 2.7 | Sy2 | |
| NGC 4388 | 40.8 ± 2.9 | 8.57 ± 0.43 | 17.9 | 120.4 ± 4.7 | 45.02 | 8.814 | 15.81 |
1.2 | Sy2 | |
| NGC 5495 | 99.8 ± 7.0 | 0.13 ± 0.02 | 15.4 | 12.5 ± 1.3 | ... | 9.301 | <0.40 | 2.4 | Sy2 | |
| NGC 5728 | 43.3 ± 3.1 | 2.27 ± 0.06 | 28.1 | 70.8 ± 2.9 | ... | 9.126 | 5.20 ± 0.20 | 2.0 | Sy2 | |
| UGC 3193 | 63.2 ± 4.4 | 3.95 ± 0.27 | 14.4 | 17.7 ± 0.7 | ... | 8.942 | <0.39 | 2.5 | U | |
| UGC 3789 | 47.4 ± 3.3 | 0.21 ± 0.02 | 14.9 | 17.6 ± 1.0 | 14.43 | 8.326 ± 0.142 | 0.26 |
2.7 | Sy2 | |
Notes. Column 1: name of galaxy. Column 2: Hubble flow distances (relative to the 3 K CMB), assuming H0 = 70 km s-1 Mpc-1 (see Sect. 2). Column 3: 33 GHz integrated flux densities with uncertainties. The errors given in those cases are formal values and do not show the real level of uncertainty. Column 4: root mean square noise level of the clean image. Column 5: NVSS integrated flux. Column 6: FIRST integrated flux. Column 7: IR (WISE, W 4) magnitude. In our analysis, a 10% uncertainty on the magnitude is assumed for those cases where the uncertainty is not given in the literature. Column 8: Swift/BAT hard X-ray fluxes (20−100 keV) with uncertainties (Litzinger et al., in prep.). Column 9: logarithm of water maser luminosity (isotropy assumed; Zhang et al. 2012, modified for H0 = 70 km s-1 Mpc-1). In our analysis, 10% uncertainty on the luminosity is assumed. Column 10: types of nuclear activity after NED; U stands for unidentified.
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