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This article has an erratum: [https://doi.org/10.1051/0004-6361/201014245e]

 

 

Table 4:

Stellar and planetary parameters of planet-bearing stars within 30 pc, as observed by XMM-Newton.

Star 		Type Dist. mV B-V P* [Fe/H] $a_{\rm pl}$ $M_{\rm pl}$ GTI Net countratea $F_{\rm X}$ $\log L_{\rm X}$ $\log \frac{L_{\rm X}}{L_{\rm bol}}$
    (pc)     (d)   (AU) ($M_{\rm J}$) (s) (cts/ks) (erg s-1 cm-2) 0.2-2 keV  

$\epsilon$ Eri

 K2.0 V 3.2 3.73 0.88 11.2 -0.10 3.39 1.55 10385 $5611.5\pm23.3$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 $0.2\pm 0.1$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

Notes. Stellar and planetary parameters taken from www.exoplanet.eu, bolometric luminosities calculated from mV with bolometric corrections from Flower (1996).
(a) PN, 0.2-2 keV. (b) MOS1 countrate given, since PN detector suffered from pile-up for this observation. (c) Data taken from Hempel et al. (2005), combined MOS countrate given, since PN detector was optically contaminated.


Source LaTeX | All tables | In the text

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