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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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