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Home All issues Volume 502 / No 2 (August I 2009) A&A, 502 2 (2009) 457-472 Full HTML
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Table B.1:

Full sample from Papers I, II and present paper, used in the correlation fits.
Source Type Distance r0 Filter Flux $\log$  $L_{\rm MIR}$ $\log$ $L_{\rm X}$ $\alpha _{\rm IX}$
    Mpc pc   mJy erg s-1 erg s-1  
(1) (2) (3) (4) (5) (6) (7) (8) (9)
Fairall 9 1.2 206 320 NEII 306 $\pm$ 10 44.51 $\pm$ 0.03 43.87 $\pm$ 0.15 -1.21
NGC 526A 1.9 81 135 NEII_1 275 $\pm$ 55 43.70 $\pm$ 0.08 43.14 $\pm$ 0.10 -1.21
SWIFT J0138.6-4001 2 108 175 PAH2 34 $\pm$ 3 43.10 $\pm$ 0.04 43.59 $\pm$ 0.30 -0.96
Mrk 590 1 112 175 NEII 106 $\pm$ 13 43.55 $\pm$ 0.06 43.61 $\pm$ 0.25 -1.06
NGC 1068 CT 14 25 * 9500 $\pm$ 475 43.80 $\pm$ 0.03 43.40 $\pm$ 0.30 -1.16
NGC 1097 L 17 30 NEII_1 28 $\pm$ 7 41.40 $\pm$ 0.11 40.80 $\pm$ 0.15 -1.22
SWIFT J0601.9-8636 2 25 45 NEII_2 72 $\pm$ 15 42.11 $\pm$ 0.08 41.92 $\pm$ 0.30 -1.10
ESO 209-G012 1.5 179 280 NEII 188 $\pm$ 26 44.22 $\pm$ 0.06 43.65 $\pm$ 0.15 -1.21
NGC 3081 1h 34 55 NEII_2 138 $\pm$ 11 42.64 $\pm$ 0.04 42.60 $\pm$ 0.30 -1.07
ESO 263-G013 2 143 225 NEII 46 $\pm$ 3 43.42 $\pm$ 0.02 43.30 $\pm$ 0.40 -1.09
NGC 3281 CT 46 75 NEII_2 1016 $\pm$ 52 43.76 $\pm$ 0.02 43.30 $\pm$ 0.15 -1.16
NGC 3393 CT 53 90 NEII_2 94 $\pm$ 5 42.90 $\pm$ 0.02 43.04 $\pm$ 0.30 -1.01
NGC 3783 1.5 43 70 NEII_1 722 $\pm$ 67 43.52 $\pm$ 0.05 43.21 $\pm$ 0.15 -1.15
NGC 4388 1h 17 30 NEII_2 375 $\pm$ 28 42.45 $\pm$ 0.03 42.24 $\pm$ 0.30 -1.11
NGC 4507 1h 51 80 NEII_1 685 $\pm$ 50 43.67 $\pm$ 0.04 43.30 $\pm$ 0.15 -1.17
NGC 4579 L 21 35 NEII_1 61 $\pm$ 21 41.88 $\pm$ 0.14 41.10 $\pm$ 0.15 -1.26
NGC 4593 1 38 65 NEII_1 382 $\pm$ 73 43.18 $\pm$ 0.08 42.93 $\pm$ 0.20 -1.13
IC 3639 CT 46 75 NEII_2 542 $\pm$ 29 43.51 $\pm$ 0.02 43.62 $\pm$ 0.50 -1.04
ESO 323-G032 1.9 68 110 PAH2 61 $\pm$ 6 42.96 $\pm$ 0.04 42.43 $\pm$ 0.40 -1.24
NGC 4941 2 17 30 NEII_1 81 $\pm$ 6 41.74 $\pm$ 0.05 41.30 $\pm$ 0.30 -1.18
NGC 4992 2 108 175 NEII 71 $\pm$ 4 43.36 $\pm$ 0.02 43.23 $\pm$ 0.30 -1.09
IRAS 13197-1627 1h 73 115 NEII_1 875 $\pm$ 46 44.07 $\pm$ 0.03 42.78 $\pm$ 0.20 -1.31
Cen A 2 3.8 7 NEII_1 1451 $\pm$ 73 41.80 $\pm$ 0.04 41.68 $\pm$ 0.15 -1.10
NGC 5135 CT 60 95 NEII_1 123 $\pm$ 12 43.06 $\pm$ 0.05 43.00 $\pm$ 0.50 -1.07
MCG-06-30-15 1.5 34 55 NEII_1 393 $\pm$ 49 43.07 $\pm$ 0.06 42.74 $\pm$ 0.20 -1.10
NGC 5728 CT 38 65 NEII_2 123 $\pm$ 10 42.69 $\pm$ 0.03 42.80 $\pm$ 0.30 -1.03
NGC 5995 2 108 170 NEII 421 $\pm$ 61 44.11 $\pm$ 0.06 43.54 $\pm$ 0.15 -1.20
ESO 138-G001 CT 38 65 NEII_2 862 $\pm$ 45 43.54 $\pm$ 0.02 43.00 $\pm$ 0.30 -1.17
NGC 6300 2 16 25 NEII_2 727 $\pm$ 38 42.69 $\pm$ 0.02 42.30 $\pm$ 0.30 -1.11
ESO 103-G035 2 57 95 NEII_2 622 $\pm$ 49 43.74 $\pm$ 0.03 43.44 $\pm$ 0.15 -1.14
ESO 141-G055 1 156 240 NEII_1 170 $\pm$ 47 44.04 $\pm$ 0.11 43.90 $\pm$ 0.15 -1.10
NGC 6814 1.5 21 35 NEII_2 96 $\pm$ 6 42.07 $\pm$ 0.02 42.12 $\pm$ 0.40 -1.07
Mrk 509 1.5 147 225 NEII 269 $\pm$ 42 44.18 $\pm$ 0.07 44.10 $\pm$ 0.15 -1.11
PKS 2048-57 1h 47 80 NEII_1 1035 $\pm$ 108 43.82 $\pm$ 0.05 42.84 $\pm$ 0.20 -1.30
PG 2130+099 1.5 274 415 NEII 179 $\pm$ 31 44.53 $\pm$ 0.07 43.65 $\pm$ 0.20 -1.24
NGC 7172 2 38 60 NEII_1 165 $\pm$ 27 42.79 $\pm$ 0.07 42.76 $\pm$ 0.40 -1.09
NGC 7213 L 25 40 NEII_1 271 $\pm$ 27 42.67 $\pm$ 0.05 42.23 $\pm$ 0.15 -1.18
3C 445 1.5 247 365 NEII 206 $\pm$ 28 44.50 $\pm$ 0.06 44.26 $\pm$ 0.15 -1.16
NGC 7314 1h 21 35 PAH2 75 $\pm$ 22 41.96 $\pm$ 0.12 42.20 $\pm$ 0.15 -1.01
NGC 7469 1.5 68 110 NEII_1 627 $\pm$ 35 43.92 $\pm$ 0.03 43.15 $\pm$ 0.10 -1.24
NGC 7674 CT 125 195 NEII 506 $\pm$ 29 44.31 $\pm$ 0.03 44.56 $\pm$ 0.50 -1.00
NGC 7679 2 73 115 NEII_1 46 $\pm$ 18 42.82 $\pm$ 0.15 42.52 $\pm$ 0.15 -1.14
Targets listed in order of increasing right ascension. In Col. (2), L = LINER and CT = Compton-thick. Column (4) lists approximate physical scale corresponding to an angular resolution limit of 0 $.\!\!^{\prime\prime}$35. * For NGC 1068, observations around 12 $\mu $m from Tomono et al. (2001) and Mason et al. (2006) were used. Refer to Table 1 and the text for other details.

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