\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}