Table 2: Measured Bondi accretion rates and jet power.
Name Flag $r_{\rm B}$ $r_{\min}$/$r_{\rm B}$ $\alpha$ KT $n_{\rm e}$ $\dot{M}_{\rm B}$ $\dot{P}_{\rm B}$ $P_{\rm j}$ ${\cal S}_{1~{\rm kpc}}$
    [pc]     [keV] [cm-3] [10 $^{-3}~M_\odot~{\rm yr}^{-1}$]       [1043 erg s-1]  
3C 028 R 19 101   $1.70\pm0.06$       <3.3 -3.26
3C 031 E 21 36   $0.82\pm0.08$       7.9 -3.53
3C 066B   69 11 $1.2_{\rm -0.3}^{+0.1}$ $0.42\pm0.08$ $\rm0.35_{-0.16}^{+0.26}$ 350 $390(\pm 31$%) 17.8 -3.72
3C 075 W 41 22   $0.57\pm0.07$       6.7 -4.19
3C 078 W 11 96   $1.19\pm0.08$       87.7 -2.74
3C 083.1   131 7 $1.6_{\rm -0.1}^{+0.4}$ $0.66\pm0.06$ $\rm0.92_{-0.48}^{+0.57}$ 2100 $1300(\pm 26$%) 4.9 -3.79
3C 084 C - -           637.0 -2.53
3C 189 W 91 17   $0.62\pm0.09$       50.5 -3.01
3C 264 E 29 26   $0.52 \pm 0.08$       18.1 -3.32
3C 270   32 9 $1.2_{\rm -0.2}^{+0.3}$ $0.55\pm0.02$ $\rm 5.4_{-3.1}^{+3.3}$ 460 $260(\pm 31\%)$ 5.9 -3.72
3C 272.1 * 30 - $0.55_{\rm -0.18}^{+0.19}$ $0.71 \pm 0.05$ $\rm0.92_{-0.47}^{+0.99}$ 85 $49(_{\rm -29 \%}^{+30 \%})$ $1.5 \pm 0.46$ -4.05
3C 274 * 117 - $0.00_{\rm -0.10}^{+0.10}$ $0.80 \pm 0.01$ $\rm0.166_{-0.032}^{+0.036}$ 240 $145(_{\rm -40 \%}^{+28 \%})$ $3.4 \pm 1.67$ -2.95
3C 293 W - -           33.6 -3.45
3C 296   32 28 $1.7_{\rm -0.2}^{+0.3}$ $0.66\pm0.03$ $\rm 42_{-29}^{+42}$ 4000 $2280(\pm 37\%)$ 11.3 -3.21
3C 317 C - -           59.4 -3.40
3C 338 * 20 - $\rm0.50_{-0.06}^{+0.07}$ $1.3\pm0.7$ $\rm0.96_{-0.29}^{+0.38}$ 55 $30.9(_{\rm -26\%}^{+34\%})$ $1.6\pm0.47$ -2.84
3C 346 E 55 94   $0.84\pm0.05$       354.9 -2.71
3C 348 R 34 339   $1.5\pm0.1$       37.7 -2.11
3C 438 R 13 815   $1.41\pm0.09$       133.8 -2.40
3C 442 W 6 17   $1.42\pm0.11$       1.0 -4.15
3C 449   18 32 $1.4_{\rm -0.2}^{+0.4}$ $0.64\pm0.08$ $18_{\rm -14}^{+15}$ 530 $302(\pm 38$%) 4.6 -4.04
3C 465   42 27 $1.4_{\rm -0.3}^{+0.1}$ $1.11\pm0.02$ $12_{\rm -4}^{+8}$ 2500 $1400(\pm 25\%)$ 38.3 -3.14

UGC 0968		 E 21 10   $0.56\pm0.04$       0.15 -4.44
UGC 5902 E 8 7   $0.44\pm0.05$       0.024 -5.39
UGC 6297   7 9 $0.9_{\rm -0.7}^{+0.1}$ $1.08\pm0.36$ $4.0_{\rm -1.5}^{+7.0}$ 21 $4.8(\pm 51\%)$ 0.067 -5.48
UGC 7203 W - -           0.33 -
UGC 7386   23 4 $1.8_{\rm -0.3}^{+0.5}$ $0.39\pm0.10$ $4.2_{\rm -3.2}^{+5.0}$ 160 $89(\pm 43\%)$ 1.5 -5.35
UGC 7629 * 36 - $0.36_{\rm -0.12}^{+0.12}$ $0.70\pm0.16$ $0.82_{\rm -0.29}^{+0.52}$ 110 $61.7(_{\rm -23 \%}^{+25 \%})$ $0.81\pm0.23$ -4.10
UGC 7760 * 17 - $0.83_{\rm -0.08}^{+0.08}$ $0.67\pm0.09$ $1.26_{\rm -0.81}^{+3.48}$ 44 $23.4(_{\rm -21 \%}^{+22 \%})$ $0.16\pm0.04$ -5.18
UGC 7797 E 10 29   $0.71\pm0.08$       0.88 -4.84
UGC 7878 * 10 - $0.31_{\rm -0.09}^{+0.09}$ $0.54\pm0.11$ $0.42_{\rm -0.15}^{+0.26}$ 47 $1.95(\pm 24\%)$ $0.030\pm0.008$ -4.02
UGC 7898   83 2.4 $1.0_{\rm -0.2}^{+0.1}$ $0.80\pm0.02$ $0.16_{\rm -0.04}^{+0.05}$ 110 $65(\pm 24\%)$ 0.34 -3.61
UGC 8745   15 22 $1.7_{\rm -0.5}^{+0.2}$ $0.54\pm0.11$ $39_{\rm -25}^{+56}$ 750 $420(\pm 45\%)$ 0.60 -4.75
UGC 9706 * 19 - $0.35_{\rm -0.21}^{+0.26}$ $0.67\pm0.09$ $0.33_{\rm -0.20}^{+0.56}$ 13 $7.08(_{\rm -40 \%}^{+43 \%})$ $0.074\pm0.026$ -3.50
UGC 9723 R 2.5 101   $0.73\pm0.07$       0.14 -5.19
NGC 1316 E 14 13   $0.54\pm0.06$       0.61 -3.94
NGC 1399   44 4 $1.0_{\rm -0.2}^{+0.1}$ $0.88\pm0.01$ $2.3_{\rm -0.8}^{+1.1}$ 490 $280(\pm 28\%)$ 0.22 -3.96
NGC 3557   52 3 $1.1_{\rm -0.5}^{+0.5}$ $0.30\pm0.09$ $1.1_{\rm -0.7}^{+1.2}$ 190 $105(\pm 41\%)$ 0.74 -4.94
NGC 4696 * 16 - $0.63_{\rm -0.30}^{+0.30}$ $0.81\pm0.05$ $1.58_{\rm -1.13}^{+4.27}$ 3.4 $25.1(_{\rm -55 \%}^{+56 \%})$ $0.79\pm0.30$ -3.97
NGC 5128 C - -           4.5 -4.61
NGC 5419 E 45 11   $0.78\pm0.11$       1.6 -3.76
IC 1459   80 2.4 $1.5_{\rm -0.2}^{+0.4}$ $0.63\pm0.03$ $0.91_{\rm -0.44}^{+0.48}$ 53 $300(\pm 24\%)$ 7.7 -4.44
IC 4296   59 8 $1.6_{\rm -0.2}^{+0.1}$ $0.62\pm0.02$ $9.7_{\rm -3.5}^{+4.5}$ 3000 $1700(\pm 20\%)$ 8.7 -3.45

NGC 0507		 * 37 - $1.1_{\rm -0.04}^{+0.04}$ $0.74\pm0.04$ $3.43_{\rm -1.70}^{+2.89}$ 450 $257(\pm 9\%)$ $10.2\pm3.37$ -3.77
Summary of the measured Bondi accretion rates and power of the FR I, CoreG, and Allen sample (marked with *). Column description: (1) name, (2) quality flag, (3) Bondi accretion radius in parsec, (4) ratio between the minimum radius reached by CHANDRA resolution $r_{\min}$ and $r_{\rm B}$, (5) the logarithmic slope of the density profile, (6) temperature at the accretion radius [keV], (7) electron number density at the accretion radius [cm-3], (8) Bondi accretion rate [ $M_\odot~{\rm yr}^{-1}$], (9) predicted Bondi accretion power [1043 erg s-1], (10) radio jet power [1043 erg s-1] (the error on $P_{\rm J}$ is assumed to be 0.4 dex, the dispersion of the Heinz et al. (2007) relation linking it to the core power except for the Allen et al. objects for which we used their published values), (11) logarithm of the surface brightness at 1 kpc, ${\cal S}_{1~{\rm kpc}}$ [counts s-1 arcsec-2].

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