\begin{table}%t2
\caption{Measured Bondi accretion rates and jet power.}\label{bondi}
%\centerline
 {\small \begin{tabular}{lcccccccccc}
\hline \hline
Name &  Flag & $r_{\rm B}$ & $r_{\min}$/$r_{\rm B}$ & $\alpha$  & $KT$ & $n_{\rm e}$ &$\dot{M}_{\rm B}$& $\dot{P}_{\rm B}$ & $P_{\rm j}$ & ${\cal S}_{1~{\rm kpc}}$ \\
 &  &\tiny{[pc]} &  & & \tiny{[keV]}       &  \tiny{[cm$^{-3}$]}  & \tiny{[10$^{-3}~M_\odot~{\rm yr}^{-1}$]} & \multicolumn{2}{c}{\tiny{$~~~~~~$[10$^{43}$ erg s$^{-1}$]}}        &  \\
\hline  
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 &  $1.2_{\rm -0.3}^{+0.1}$ & $0.42\pm0.08$ &$\rm 0.35_{-0.16}^{+0.26}$& 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 &  $1.6_{\rm -0.1}^{+0.4}$ & $0.66\pm0.06$ & $\rm 0.92_{-0.48}^{+0.57}$& 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  &  -- & $0.55_{\rm -0.18}^{+0.19}$& $0.71 \pm 0.05$ & $\rm 0.92_{-0.47}^{+0.99}$   &   85  & $49(_{\rm -29 \%}^{+30 \%})$& $1.5 \pm 0.46$& --4.05 \\
3C~274   & * & 117  &  -- & $0.00_{\rm -0.10}^{+0.10}$& $0.80 \pm 0.01$ & $\rm 0.166_{-0.032}^{+0.036}$&   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  &  -- &$\rm 0.50_{-0.06}^{+0.07}$&$1.3\pm0.7$ &$\rm 0.96_{-0.29}^{+0.38}$  & 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 \\
\noalign{\smallskip}\hline\noalign{\smallskip}	                  			 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\\
\noalign{\smallskip}\hline\noalign{\smallskip}      				 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\\
\hline
\end{tabular}}
\smallskip	
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 [$10^{43}$~erg~s$^{-1}$], (10) radio jet power [10$^{43}$~erg~s$^{-1}$] (the error on $P_{\rm J}$ is assumed to be 0.4~dex, the dispersion of the \citet{heinz07} 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$^{-2}$].
\end{table}