\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}