Table A.3
Summary of the Palomar LLAGN sample with nuclear radio detections at 15 GHz in high resolution (mainly from this paper, and Nagar et al. 2005), with a compilation of mass and X-ray luminosity from the literature (references listed at the end of the table).
| Name | Log LR (erg s−1) | Log LX (erg s−1) | Log M (M⊙) | Dist (Mpc) | Ref |
|---|---|---|---|---|---|
| (1) | (2) | (3) | (4) | (5) | (6) |
| NGC266 | 38.46 | 40.77 | 8.60 | 62.4 | 5 |
| NGC315 | 40.56 | 41.77 | 9.22 | 65.8 | 2 |
| NGC410 | 37.81 | 40.71 | 9.19 | 70.6 | 2 |
| NGC660 | 38.20 | 38.32 | 7.30 | 11.8 | 4 |
| NGC1055 | 35.72 | 38.38 | 6.25 | 12.6 | 4 |
| NGC1167 | 39.54 | 39.60 | 8.47 | 65.3 | 1 |
| NGC1275 | 41.42 | 43.40 | 8.86 | 70.1 | 6 |
| NGC2273 | 37.77 | 40.93 | 7.63 | 28.4 | 1 |
| NGC2655 | 37.81 | 40.89 | 7.79 | 24.4 | 1 |
| NGC2681 | 36.03 | 39.27 | 6.94 | 13.3 | 2 |
| NGC2683 | 35.42 | 38.21 | 7.34 | 5.7 | 7 |
| NGC2787 | 37.33 | 38.80 | 8.31 | 13.0 | 2 |
| NGC2841 | 36.45 | 39.22 | 8.52 | 12.0 | 2 |
| NGC3031 | 37.58 | 39.48 | 7.82 | 3.6 | 1 |
| NGC3079 | 38.55 | 40.26 | 8.08 | 20.4 | 1 |
| NGC3147 | 38.38 | 41.49 | 8.50 | 40.9 | 1 |
| NGC3169 | 37.68 | 41.35 | 8.16 | 19.7 | 8 |
| NGC3226 | 37.69 | 40.80 | 8.22 | 23.4 | 2 |
| NGC3227 | 37.43 | 41.64 | 7.43 | 20.6 | 1 |
| NGC3414 | 37.41 | 39.86 | 8.67 | 24.9 | 2 |
| NGC3516 | 37.55 | 42.42 | 8.07 | 38.9 | 1 |
| NGC3607 | 37.06 | 38.76 | 8.62 | 19.9 | 2 |
| NGC3627 | 35.93 | 39.41 | 7.23 | 6.6 | 2 |
| NGC3628 | 36.20 | 39.94 | 6.18 | 7.7 | 2 |
| NGC3718 | 37.74 | 41.06 | 7.77 | 17.0 | 5 |
| NGC3735 | 37.08 | 40.53 | 7.51 | 41.0 | 1 |
| NGC3945 | 37.21 | 39.12 | 8.19 | 22.5 | 2 |
| NGC3982 | 36.47 | 39.78 | 6.05 | 17.0 | 1 |
| NGC3998 | 38.68 | 41.32 | 9.23 | 21.6 | 2 |
| NGC4036 | 36.82 | 38.12 | 8.45 | 24.6 | 2 |
| NGC4051 | 36.40 | 41.35 | 6.49 | 17.0 | 1 |
| NGC4111 | 35.99 | 40.36 | 7.62 | 17.0 | 2 |
| NGC4138 | 36.89 | 41.28 | 7.17 | 17.0 | 1 |
| NGC4143 | 37.23 | 40.03 | 8.34 | 17.0 | 8 |
| NGC4151 | 37.97 | 43.01 | 6.68 | 20.3 | 1 |
| NGC4168 | 37.18 | 39.30 | 8.10 | 16.8 | 1 |
| NGC4169 | 37.74 | 40.84 | 8.09 | 50.4 | 1 |
| NGC4203 | 37.21 | 40.37 | 7.89 | 9.7 | 3 |
| NGC4258 | 36.33 | 40.90 | 7.62 | 6.8 | 3 |
| NGC4261 | 39.82 | 41.07 | 9.26 | 35.1 | 2 |
| NGC4278 | 38.17 | 39.23 | 8.88 | 9.7 | 2 |
| NGC4374 | 38.96 | 39.53 | 9.25 | 16.8 | 2 |
| NGC4388 | 37.05 | 41.85 | 6.56 | 16.8 | 1 |
| NGC4395 | 34.59 | 40.08 | 4.07 | 3.6 | 1 |
| NGC4450 | 37.01 | 40.35 | 7.42 | 16.8 | 3 |
| NGC4472 | 37.27 | 39.85 | 9.12 | 16.8 | 1 |
| NGC4486 | 40.14 | 40.82 | 9.42 | 16.8 | 2 |
| NGC4548 | 36.78 | 39.79 | 7.03 | 16.8 | 8 |
| NGC4552 | 38.47 | 39.25 | 8.81 | 16.8 | 2 |
| NGC4565 | 36.80 | 41.32 | 7.43 | 9.7 | 1 |
| NGC4579 | 38.15 | 41.17 | 7.86 | 16.8 | 2 |
| NGC4589 | 38.28 | 38.91 | 8.54 | 30.0 | 2 |
| NGC4636 | 36.92 | 39.03 | 8.32 | 17.0 | 2 |
| NGC4736 | 35.80 | 38.59 | 7.00 | 4.3 | 2 |
| NGC4750 | 37.02 | 40.08 | 7.43 | 26.1 | 5 |
| NGC4772 | 37.20 | 39.85 | 7.62 | 16.3 | 5 |
| NGC5033 | 36.94 | 42.64 | 7.67 | 18.7 | 1 |
| NGC5194 | 35.43 | 39.30 | 6.66 | 7.7 | 1 |
| NGC5273 | 36.18 | 41.58 | 5.99 | 21.3 | 1 |
| NGC5363 | 38.54 | 39.78 | 8.57 | 22.4 | 2 |
| NGC5746 | 37.32 | 40.22 | 8.29 | 29.4 | 2 |
| NGC5813 | 37.51 | 38.80 | 8.68 | 28.5 | 2 |
| NGC5838 | 37.37 | 39.20 | 8.92 | 28.5 | 2 |
| NGC5846 | 37.96 | 40.81 | 8.67 | 28.5 | 2 |
| NGC5866 | 37.47 | 38.29 | 7.92 | 15.3 | 2 |
| NGC6482 | 37.32 | 39.33 | 9.27 | 52.3 | 2 |
| NGC6500 | 39.37 | 40.11 | 8.44 | 39.7 | 8 |
| NGC6951 | 36.44 | 39.48 | 7.29 | 24.1 | 1 |
| NGC7479 | 37.66 | 40.45 | 7.72 | 32.4 | 1 |
| NGC7743 | 37.03 | 37.85 | 6.50 | 24.4 | 1 |
Notes. Columns are: (1) galaxy name; (2) logarithmic value of radio luminosity at 15 GHz (in erg s−1) with the VLA; (3) logarithmic value of X-ray luminosity at 2–10 keV (in erg s−1), taken from Literature (reference given in Col. 6); (4) logarithmic value of black hole mass (in M⊙), estimated from stellar velocity dispersions reported in Ho et al. (2009) using the empirical relation given in McConnell et al. (2011); (5) distance to the source in Mpc; (6) literature references for the X-ray luminosity at 2–10 KeV range quoted in Col. 3.
References for X-ray luminosity. 1: Akylas & Georgantopoulos (2009), 2: González-Martín et al. (2009), 3: Terashima et al. (2002), 4: Filho et al. (2004), 5: Younes et al. (2011), 6: Allen et al. (2001), 7: Panessa et al. (2006), 8: Terashima & Wilson (2003).
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