\begin{table}%t4
\par
%\centering
\par
\caption{\label{counts}Stellar and planetary parameters of planet-bearing stars within 30 pc, as observed by XMM-Newton.}
      \begin{tabular}{l l r r r r r l r r r r r r}
    \hline
    \hline
    \noalign{\smallskip}
       Star & Type & Dist. & $m_V$ & $B-V$ & $P_*$ & [Fe/H] & $a_{\rm pl}$ & $M_{\rm pl}$ & GTI &  Net countrate\tablefootmark{a} & $F_{\rm X}$ & $\log L_{\rm X}$ & $\log \frac{L_{\rm X}}{L_{\rm bol}}$\\
                                                                           & & (pc) & & & (d) & & (AU) & ($M_{\rm J}$) & (s) &  (cts/ks) & (erg~s$^{-1}$~cm$^{-2}$) & 0.2--2~keV & \\
\par
    \hline
                                   $\epsilon$ Eri & K2.0 V      &  3.2 &   3.73 & 0.88 &   11.2 & --0.10 &  3.39 &  1.55 & 10385 &  $5611.5\pm23.3$\tablefootmark{b} &   1.38E-11 & $28.22\pm0.12$ & --4.88\\
                                                GJ 674 & M2.5   &  4.5 &   9.38 & 1.53 &   35.0 & --0.28 &  0.04 &  0.04 & 15183 &  $1102.6\pm 8.6$ &   2.16E-12 & $27.73\pm0.12$ & --3.80\\
                                           GL 876 & M4.0 V      &  4.7 &  10.17 & 1.67 &   41.0 & --0.12 &  0.02 &  0.02 & 23436 &    $48.9\pm 1.5$ &   1.13E-13 & $26.48\pm0.13$ & --5.11\\
                                                 VB 10 & M8.0 V      &  5.8 &   9.91 & 0.00 & -- &  0.00 &  0.36 &  6.40 & 10810 &    $23.2\pm 1.5$ &   4.91E-14 & $26.30\pm0.14$ & --1.79\\
                                                     GJ 317 & M3.5   &  9.2 &  12.00 & 1.53 & -- & --0.23 &  0.95 &  1.20 & 11245 &    $14.3\pm 1.5$ &   3.30E-14 & $26.52\pm0.14$ & --4.57\\
                                         HD 62509 & G5.0 IV-V   & 10.3 &   1.15 & 1.00 &  130.0 &  0.19 &  1.69 &  2.90 & 28759 &    $31.2\pm 1.1$ &   1.01E-13 & $27.11\pm0.13$ & --6.63\\
                                            GL 86 & K1.0 V      & 11.0 &   7.40 & 0.77 &   31.0 & --0.24 &  0.11 &  4.01 & 13071 &   $116.8\pm 3.1$ &   2.94E-13 & $27.63\pm0.12$ & --5.04\\
                                           55 Cnc & G8.0 V      & 13.0 &   5.95 & 0.87 &   42.7 &  0.29 &  0.04 &  0.03 &  8505 &    $18.6\pm 1.6$ &   5.77E-14 & $27.07\pm0.14$ & --6.36\\
                                           47 UMa & G0.0 V      & 14.0 &   5.10 & 0.56 &   74.0 &  0.00 &  2.11 &  2.60 &  6196 &     $2.6\pm 0.7$ &   1.07E-14 & $26.40\pm0.21$ & --7.34\\
                                           51 Peg & G5.0 V      & 14.7 &   5.49 & 0.67 &   37.0 &  0.20 &  0.05 &  0.47 & 25299 &     $0.4\pm 0.2$ &   1.70E-15 & $26.28\pm0.18$ & --7.37\\
                                       $\tau$ Boo & M8.0 V      & 15.0 &   4.50 & 0.48 &    3.3 &  0.28 &  0.05 &  3.90 & 38251 &  $1252.1\pm 5.7$ &   3.21E-12 & $28.94\pm0.12$ & --6.14\\
                                             HD 160691 & G3.0 IV-V   & 15.3 &   5.15 & 0.70 & -- &  0.28 &  0.09 &  0.04 &  7046 &     $3.6\pm 1.2$ &   1.06E-14 & $26.47\pm0.16$ & --7.36\\
                                             HD 190360 & G6.0 IV     & 15.9 &   5.71 & 0.73 & -- &  0.24 &  0.13 &  0.06 &  2888 &     $2.2\pm 1.4$ &   5.23E-15 & $26.20\pm0.21$ & --7.45\\
                                         HD 99492 & F7.0 V      & 18.0 &   7.57 & 1.01 &   45.0 &  0.36 &  0.12 &  0.11 & 19928 &     $7.1\pm 0.6$ &   2.44E-14 & $26.98\pm0.15$ & --5.97\\
                                                14 Her & K0.0 V      & 18.1 &   6.67 & 0.90 & -- &  0.43 &  2.77 &  4.64 &  5532 &    $14.6\pm 2.9$ &   3.25E-14 & $27.11\pm0.14$ & --6.33\\
                                             HD 154345 & G8.0 V      & 18.1 &   6.74 & 0.76 & -- & --0.11 &  4.19 &  0.95 &  3845 &    $18.6\pm 2.4$ &   5.46E-14 & $27.33\pm0.16$ & --6.03\\
                                              HD 27442 & K2.0 III    & 18.1 &   4.44 & 1.08 & -- &  0.20 &  1.18 &  1.28 &  4636 &     $3.7\pm 1.3$ &   1.23E-14 & $26.68\pm0.18$ & --7.72\\
                                      $\beta$ Pic & A6.0 V      & 19.3 &   3.86 & 0.17 &    0.7 &  0.00 &  8.00 &  8.00 & 54896 &     $0.2\pm 0.1$\tablefootmark{c} &   6.00E-16 & $25.40\pm0.15$ & --9.09\\
                                             HD 189733 & K1.5   & 19.3 &   7.67 & 0.93 &   13.4 & --0.03 &  0.03 &  1.13 & 36271 &   $110.3\pm 1.8$ &   4.11E-13 & $28.26\pm0.12$ & --4.84\\
                                              HD 217107 & G8.0 IV     & 19.7 &   6.18 & 0.72 &   37.0 &  0.37 &  0.07 &  1.33 &  5576 & $<$6.0 & $<$1.55E-14 & $<$26.86 & $<$--6.79\\
                                        HD 195019 & G3.0 IV-V   & 20.0 &   6.91 & 0.64 &   22.0 &  0.08 &  0.14 &  3.70 &  8333 &     $2.8\pm    0.8$ &   6.44E-15 & $26.49\pm0.17$ & --6.86\\
                                               16 Cyg B & G2.5 V      & 21.4 &   6.20 & 0.66 &   31.0 &  0.08 &  1.68 &  1.68 & 10768 & $<$1.6 & $<$5.42E-15 & $<$26.47 & $<$--7.22\\
                                                   HD 164922 & K0.0 V      & 21.9 &   7.01 & 0.80 & -- &  0.17 &  2.11 &  0.36 &  6955 & $<$3.5 & $<$1.21E-14 & $<$26.84 & $<$--6.59\\
                                               HD 4308 & G0.0 V      & 21.9 &   6.54 & 0.65 & -- & --0.31 &  0.11 &  0.05 &  7837 &     $2.1\pm    0.7$ &   7.89E-15 & $26.66\pm 0.19$ & --6.02\\
                                                  HD 114783 & K0.0   & 22.0 &   7.57 & 0.93 & -- &  0.33 &  1.20 &  0.99 &  3583 &     $2.1\pm    1.5$ &   6.72E-15 & $26.59\pm 0.19$ & --6.66\\
                                             HD 216437 & G4.0 IV-V   & 26.5 &   6.06 & 0.63 & -- &  0.00 &  2.70 &  2.10 &  3329 &     $8.2\pm    1.9$ &   1.89E-14 & $27.20\pm 0.18$ & --6.73\\
                                                   HD 20367 & G0.0   & 27.0 &   6.41 & 0.52 & -- &  0.10 &  1.25 &  1.07 &  8861 &  $1404.8\pm   12.6$ &   2.76E-12 & $29.38\pm 0.12$ & --4.40\\
                                             HD 114386 & K3.0 V      & 28.0 &   8.80 & 0.90 & -- &  0.00 &  1.62 &  0.99 &  3601 &     $2.7\pm    1.2$ &   7.19E-15 & $26.83\pm 0.21$ & --6.13\\
                                              HD 52265 & K0.0 III    & 28.0 &   6.30 & 0.54 & -- &  0.11 &  0.49 &  1.13 &  6954 &     $5.6\pm    1.0$ &   1.82E-14 & $27.23\pm 0.17$ & --6.92\\
                                         HD 75289 & K3.0 V      & 28.9 &   6.35 & 0.58 &   16.0 &  0.29 &  0.05 &  0.42 &  6681 &     $3.0\pm    0.7$ &   1.21E-14 & $27.09\pm 0.20$ & --6.75\\
                                         HD 93083 & K2.0 V      & 28.9 &   8.33 & 0.94 &   48.0 &  0.15 &  0.48 &  0.37 &  7789 &     $7.4\pm    1.3$ &   1.67E-14 & $27.22\pm 0.16$ & --6.79\\
                                        HD 102195 & K0.0 V      & 29.0 &   8.06 & 0.83 &   12.0 &  0.05 &  0.05 &  0.45 & 13043 &   $145.9\pm    3.4$ &   2.87E-13 & $28.46\pm 0.12$ & --4.81\\
                                              HD 111232 & G8.0 V      & 29.0 &   7.61 & 0.68 &   30.7 & --0.36 &  1.97 &  6.80 &  6996 & $<$3.2 & $<$9.72E-15 & $<$26.99 & $<$--6.41\\
                                              HD 70642 & G0.0 V      & 29.0 &   7.18 & 0.71 & -- &  0.16 &  3.30 &  2.00 & 10935 &     $3.0\pm    0.7$ &   6.68E-15 & $26.83\pm 0.17$ & --8.08\\
                                        HD 130322 & K0.0 V      & 30.0 &   8.05 & 0.78 &    8.7 & --0.02 &  0.09 &  1.08 &  4194 &    $16.7\pm    2.2$ &   3.87E-14 & $27.62\pm 0.16$ & --5.66\\
              \hline
\end{tabular}
\tablefoot{Stellar and planetary parameters taken from \protect\url{www.exoplanet.eu}, bolometric luminosities calculated from $m_V$ with bolometric corrections from \cite{flower1996}.\\
\tablefoottext{a}{PN, 0.2--2~keV.}
\tablefoottext{b}{MOS1 countrate given, since PN detector suffered from pile-up for this observation.}
\tablefoottext{c}{Data taken from \cite{HempelRobrade2005}, combined MOS countrate given, since PN detector was optically contaminated.}}
\vspace*{4mm}
\end{table}