\begin{table}%t3
\caption{\label{param}Stellar parameters derived for the 23 Kepler asteroseismic targets in the KIC Catalogue and 13 other stars in 
Kepler field of view, but not yet selected as mission targets.} 
%%\centering

\par
\begin{tabular}{r r r r c r c r c r r}                       
\hline            
\hline \noalign{\smallskip}           
HIP~     & KIC~~~~ &  $V$\tablefootmark{a}~~  & Plx\tablefootmark{b}~~~~ &Sp.     & $T_{\rm eff}$~~~~      & $\log g$   & $v~\sin i$   & HJD & $RV$~~~~~~ & $\log L/L_\odot$\tablefootmark{c}\\
         &         & (mag)& (mas)~~~~  &Type    & (K)~~~~           &            & (km/s) & +2~450~000    &  (km/s)~~~~ &            \\
\hline
\multicolumn{11}{c}{Kepler asteroseismic targets}\\
92247    &     11013201 &  9.24 & 4.64~$\pm$~0.79   &	...     &  7200~$\pm$~200  & 3.5~$\pm$~0.2 & 100 & 4309.492 &  $-$8.3~$\pm$~2.6 & 0.87$_{-0.18}^{+0.16}$ \\
92259    &     10187831 &  9.47 & 3.29~$\pm$~0.77   & A7~$\pm$~3 &  7100~$\pm$~200  & 3.0~$\pm$~0.5 & 120 & 4310.465 & $-$22.7~$\pm$~2.6 & 1.11$_{-0.25}^{+0.20}$ \\
92637    &     10960750 &  9.83 & $-0.70~\pm$~0.85 & O9~$\pm$~2 & 19900~$\pm$~1400 & 3.8~$\pm$~0.2 & 230 & 4307.480 & $-$22.0~$\pm$~2.8 & 1.38$_{-0.40}^{+0.28}$  \\
93070    &      3830233 &  9.36 & 2.61~$\pm$~0.93   &	... 	      &  8000~$\pm$~500  & 4.2~$\pm$~0.2 & 200 & 4306.580 &    13.4~$\pm$~3.2 & ...~~~~~ \\
93522    &      8740371 & 10.14 & 0.12~$\pm$~1.     & A7~$\pm$~2 &  9100~$\pm$~400  & 3.7~$\pm$~0.2 &   5 & 4308.483 &     1.2~$\pm$~0.4 & ...~~~~~ \\
93941\tablefootmark{1}&      6848529 & 10.64 & 5.79~$\pm$~1.03   & B2$\pm$~2   & 19300~$\pm$~1000 & 3.8~$\pm$~0.2 &  10 & 4270.370 & $-$14.3~$\pm$~3.0 & 0.85$_{-0.19}^{+0.16}$ \\
~~~$''$~~~ &~~~$''$~~~ &~~~$''$~~~&~~~$''$~~ &~~~$''$~~   &~~~$''$~~  &~~~$''$~~~ & $''$ & 5017.515 & $-$21.3~$\pm$~2.9 & ...~~~~~  \\
93943    &     12250891 &  9.70 &  5.26~$\pm$~1.58  &  ...              &  7400~$\pm$~200  & 3.4~$\pm$~0.5 &  20 & 4311.492 & $-$13.6~$\pm$~0.3 & 0.57$_{-0.33}^{+0.25}$ \\
94670    &      7599132 &  9.30 &  1.27~$\pm$~0.90  & B9~$\pm$~2 & 11600~$\pm$~500  & 4.2~$\pm$~0.2 &  50 & 4308.354 & $-$57.2~$\pm$~1.8 & ...~~~~~ \\
94809    &      6769635 &  9.32 &  3.54~$\pm$~0.72  &	... 	      &  7200~$\pm$~400  & 3.9~$\pm$~0.5 & 150 & 4290.393 &     5.8~$\pm$~4.4 & 1.10$_{-0.22}^{+0.18}$ \\
95092    &     11134456 &  9.83 &  2.62~$\pm$~0.87  &	... 	      &  8300~$\pm$~400  & 3.5~$\pm$~0.3 &  80 & 4307.546 & $-$11.2~$\pm$~2.1 & 1.19$_{-0.37}^{+0.27}$ \\
95174    &      5786771 &  9.08 &  1.91~$\pm$~0.76  & A2~$\pm$~3 & 10700~$\pm$~500  & 4.2~$\pm$~0.2 & 200 & 4306.520 & $-$21.7~$\pm$~12.1 & 1.97$_{-0.46}^{+0.31}$ \\
95495    &     11762256 &  9.23 &  3.91~$\pm$~0.75  &	... 	      &  7000~$\pm$~200  & 3.5~$\pm$~0.5 &  90 & 4308.542 & $-$43.9~$\pm$~1.8 & 1.04$_{-0.20}^{+0.17}$ \\
96210\tablefootmark{2}&     6128830  &  9.20 &  0.62~$\pm$~0.74  & B6~$\pm$~2 & 12600~$\pm$~600  & 3.5~$\pm$~0.3 &  15 & 4310.392 &     6.6~$\pm$~1.0 & \\
96277    &     10604429 &  9.93 &  2.70~$\pm$~1.11  &	... 	      &  7200~$\pm$~200  & 3.5~$\pm$~0.5 &  60 & 4278.437 &  $-$3.1~$\pm$~1.8 & 1.11$_{-0.48}^{+0.32}$ \\
~~~$''$~~~ &~~~$''$~~~ &~~~$''$~~~&~~~$''$~~ & &~~~$''$~~~ &~~~$''$~~~ &$''$ & 4313.459 &     0.7~$\pm$~1.2 & ...~~~~~ \\
~~~$''$~~~ &~~~$''$~~~ &~~~$''$~~~&~~~$''$~~ & &~~~$''$~~~ &~~~$''$~~~ &$''$ & 4361.440 &  $-$0.8~$\pm$~1.6 & ...~~~~~ \\
96299~A &      3858884 &  9.25 &  2.49~$\pm$~1.06  &  ...             & ...~~~~       & ...                    &  70 & 4290.556 &  $-$7.8~$\pm$~1.2 & ...~~~~~ \\  
96299~B &~~~$''$~~~ &~~~$''$~~~&~~~$''$~~ & ... & ...~~~~       & ... &...         & 4290.556 &    45.1~$\pm$~1.3 & ...~~~~~ \\  
96762    &      4276892 & 9.13 &  2.71~$\pm$~0.76   & B9~$\pm$~1 & 10800~$\pm$~600  & 4.1~$\pm$~0.2 &  10 & 4309.399 &    16.5~$\pm$~1.1 & 1.61$_{-0.31}^{+0.23}$ \\
97486    &      9663677 & 9.98 &  2.51~$\pm$~0.87   &	... 	      &  8000~$\pm$~300  & 3.9~$\pm$~0.4 & 160 & 4312.533 &  $-$0.8~$\pm$~4.8 & 1.17$_{-0.39}^{+0.28}$  \\
97582    &      7978223 & 9.22 &  4.12~$\pm$~0.86   &	... 	      &  7100~$\pm$~200  & 3.6~$\pm$~0.5 &  90 & 4270.494 &     3.6~$\pm$~3.5 & 0.99$_{-0.22}^{+0.18}$ \\
~~~$''$~~~ &~~~$''$~~~&~~~$''$~~~ &~~~$''$~~~& &~~~$''$~~~ &~~~$''$~~~ &$''$ & 4361.495 &	7.1~$\pm$~6.7 & ...~~~~~ \\
~~~$''$~~~ &~~~$''$~~~&~~~$''$~~~ &~~~$''$~~~& &~~~$''$~~~ &~~~$''$~~~ &$''$ & 4312.593 &	2.6~$\pm$~2.9 & ...~~~~~ \\
97254    &      4581434 &  9.07 &  1.65~$\pm$~0.80  & A2~$\pm$~3 & 10200~$\pm$~200  & 4.2~$\pm$~0.2 & 200 & 4306.403 &  $-$4.3~$\pm$~6.2  & 2.08$_{-0.60}^{+0.36}$ \\
97724    &      4681323 &  9.05 &  1.85~$\pm$~0.76  &	... 	      &  8900~$\pm$~400  & 3.5~$\pm$~0.2 &  90 & 4308.590 &  $-$14.8~$\pm$~4.0 & 1.87$_{-0.48}^{+0.32}$ \\ 
98037    &      5304891 &  9.16 &  1.78~$\pm$~0.74  & B6~$\pm$~2 & 13100~$\pm$~700  & 3.9~$\pm$~0.2 & 180 & 4309.550 &  $-$30.9~$\pm$~20.4 & 2.21$_{-0.49}^{+0.32}$ \\
98160    &      8389948 &  9.16 &  2.79~$\pm$~0.75  &	... 	      & 10000~$\pm$~300  & 4.0~$\pm$~0.2 & 130 & 4307.418 &  $-$31.7~$\pm$~5.4 & 1.50$_{-0.29}^{+0.23}$  \\
\hline 
\multicolumn{11}{c}{Stars not selected as Kepler targets}\\
91178    &              &  9.10 &  1.79~$\pm$~0.75  & A2~$\pm$~2 &  9900~$\pm$~200  & 4.0~$\pm$~0.1 & 110 & 4306.463 & $-$11.8~$\pm$~1.4 & 1.96$_{-0.49}^{+0.32}$ \\     
93924    &              &  9.09 &  1.47~$\pm$~0.78  &	... 	      & 10400~$\pm$~300  & 4.2~$\pm$~0.2 & 150 & 4306.352 & $-$39.6~$\pm$~6.5 & ...~~~~~ \\
94137    &              &  9.83 &  2.17~$\pm$~0.88  &	... 	      &  7200~$\pm$~200  & 4.0~$\pm$~0.4 &  50 & 4311.580 & $-$28.0~$\pm$~1.2 & 1.37$_{-0.47}^{+0.32}$ \\
95069    &              &  9.05 &  2.70~$\pm$~1.09  & A1~$\pm$~2 & 12300~$\pm$~700  & 4.0~$\pm$~0.2 & 200 & 4307.372 & $-$13.8~$\pm$~1.7 & 1.77$_{-0.47}^{+0.31}$ \\
95506    &              &  9.15 &  3.66~$\pm$~0.69  & A1~$\pm$~2 & 10200~$\pm$~400  & 4.0~$\pm$~0.3 & 200 & 4309.345 & $-$22.8~$\pm$~4.6 & 1.26$_{-0.20}^{+0.17}$ \\
96061\tablefootmark{3}&              &  9.64 &  1.75~$\pm$~6.82  & A3~$\pm$~3 & 11300~$\pm$~500  & 4.2~$\pm$~0.2 &  70 & 4285.370 & $-$22.0~$\pm$~2.3 & ...~~~~~ \\
~~~$''$~~~ &~~~~~~~~&~~~$''$~~~ &~~~$''$~~~& &~~~$''$~~~ &~~~$''$~~~ &$''$ & 5108.346  &  $-$20.5~$\pm$~1.6 & \\
96066    &              &  8.80 &  4.04~$\pm$~2.13  & A1~$\pm$~3 & 10400~$\pm$~300  & 4.1~$\pm$~0.2 &  50 & 5103.450 &  $-$28.5~$\pm$~2.2   & ...~~~~~ \\
96343    &              &  9.70 &  3.80~$\pm$~0.91  & B9~$\pm$~3 & 11700~$\pm$~600  & 4.1~$\pm$~0.2 & 160 & 4311.365 &  $-$4.5~$\pm$~3.1 & 1.14$_{-0.26}^{+0.21}$ \\
96776    &              &  9.52 &  1.60~$\pm$~0.74  &	... 	      &  7600~$\pm$~200  & 4.5~$\pm$~0.5 & 200 & 4310.541 &  $-$7.7~$\pm$~3.6 & 1.80$_{-0.56}^{+0.35}$ \\
98486    &              &  9.59 &  1.20~$\pm$~0.90  &	... 	      & 10300~$\pm$~400  & 4.0~$\pm$~0.2 &  70 & 4308.409 &  $-$23.8~$\pm$~3.2 &  ...~~~~~ \\
98551~A &              & 10.36 &  2.17~$\pm$~1.18  & ... 	      & ...~~~~		 & ...  	   &  70 & 4313.538 & $-$23.4~$\pm$~3.3    &  ...~~~~~ \\
98551~B &              &~~~$''$~~~ &~~~$''$~~~& ... & ...~~~~ & ... & ...    & 4313.538 &    44.6~$\pm$~2.0 &  \\
98814    &              & 10.10 &  1.45~$\pm$~0.91  & B6~$\pm$~3  & 13900~$\pm$~1000 & 3.9~$\pm$~0.3 &  40 & 4313.372 & $-$40.7~$\pm$~3.5 &  ...~~~~~ \\    
\hline
\end{tabular}\\
\tablefoot{
\tablefoottext{a}{$V$ magnitude from the Hipparcos main catalogue \citep{esa97}.}
\tablefoottext{b}{Parallax from \citet{vanLeeuwen}.}
\tablefoottext{c}{Luminosity in solar units computed only for those stars with relative parallax errors $\le$50$\%$.}
\tablefoottext{1}{He-weak. Gravity in disagreement with the position on the HR diagram.}
\tablefoottext{2}{HgMn star.}
\tablefoottext{3}{Based on the proper motions \citep{esa97} and radial velocities, we suppose that HIP~96061 is likely a physical binary with HIP~96066 with a separation of ${\approx}$11\farcs 5.}}
 \vspace*{1.3mm}  \end{table}