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Home All issues Volume 507 / No 1 (November III 2009) A&A, 507 1 (2009) 523-530 Full HTML
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Table 2:

Stellar parameters and iron abundance of host stars of transiting planets.
Star $T_{\rm eff}$ [K] ${\log}~g~$(cgs) $\xi_{\rm t}$ [km s-1] [Fe/H] N(Fe I, Fe II) $\sigma({\rm Fe~I, Fe~II})$ Source
CoRoT-Exo-2 $5608\pm37$ $4.71\pm0.20$ $1.49\pm0.06$ $0.07\pm0.04 $ 26, 9 0.03, 0.09 this work
HAT-P-1 $6076\pm27$ $4.47\pm0.07$ $1.17\pm0.05$ $ 0.21\pm0.03$ 21, 10 0.02, 0.03 this work
HAT-P-2 $6951\pm181$ $4.45\pm0.08$ $1.61\pm0.33$ $0.49\pm0.12$ 14, 8 0.06, 0.03 this work
HAT-P-4 $6054\pm 60$ $4.17\pm0.28$ $1.59\pm0.09$ $0.35\pm0.08$ 30, 9 0.06, 0.12 this work
HAT-P-6 $6855\pm111$ $4.69\pm0.20$ $2.85\pm1.15$ $-0.08\pm0.11$ 21, 9 0.07, 0.07 this work
HAT-P-7 $6525\pm 61$ $4.09\pm0.08$ $1.78\pm0.14$ $0.31\pm0.07$ 33, 10 0.06, 0.03 this work
HD 17156 $6084\pm 29$ $4.33\pm0.05$ $1.47\pm0.05$ $0.23\pm0.04$ 30, 10 0.03, 0.02 this work
HD 80606 $5574\pm72$ $4.46\pm0.20$ $1.14\pm0.09$ $0.32\pm0.09$ 38, 5 0.07, 0.08 Santos et al. (2004)
HD 149026 $6162\pm41$ $4.37\pm0.10$ $1.41\pm0.07$ $0.36\pm0.05$ 23, 9 0.04, 0.04 this work
HD 189733 $5050\pm50$ $4.53\pm0.14$ $0.95\pm0.07$ $-0.03\pm0.04$ -, - -, - Bouchy et al. (2005)
HD 209458 $6117\pm26$ $4.48\pm0.08$ $1.40\pm0.06$ $0.02\pm0.03$ -, - -, - Santos et al. (2004)
OGLE-TR-10 $6075\pm86$ $4.54\pm0.15$ $1.45\pm0.14$ $0.28\pm0.10$ 33, 11 0.08, 0.06 Santos et al. (2006b)
OGLE-TR-56 $6119\pm62$ $4.21\pm0.19$ $1.48\pm0.11$ $0.25\pm0.08$ 31, 9 0.06, 0.08 Santos et al. (2006b)
OGLE-TR-111 $5044\pm83$ $4.51\pm0.36$ $1.14\pm0.10$ $0.19\pm0.07$ 31, 7 0.07, 0.18 Santos et al. (2006b)
OGLE-TR-113 $4804\pm106$ $4.52\pm0.26$ $0.90\pm0.18$ $0.15\pm0.10$ 30, 5 0.10, 0.09 Santos et al. (2006b)
OGLE-TR-132 $6411\pm179$ $4.86\pm0.14$ $1.46\pm0.36$ $0.43\pm0.18$ -, - -,- Bouchy et al. (2004)
OGLE-TR-182 $5924\pm64$ $4.47\pm0.18$ - $0.37\pm0.08$ -, - -, - Pont et al. (2008)
OGLE-TR-211 $6325\pm91$ $4.22\pm0.17$ $1.63\pm0.21$ $0.11\pm0.10$ -, - -, - Udalski et al. (2008)
TrES-1 $5226\pm38$ $4.40\pm0.10$ $0.90\pm0.05$ $0.06\pm0.05$ 36, 7 0.04, 0.05 Santos et al. (2006b)
TrES-2 $5795\pm73$ $4.30\pm0.13$ $0.79\pm0.12$ $ 0.06\pm0.08$ 20, 9 0.06, 0.05 this work
TrES-3 $5502\pm157$ $4.44\pm0.22$ $1.00\pm0.30$ $-0.10\pm0.19$ 20, 8 0.14, 0.07 this work
TrES-4 $6293\pm 96$ $4.20\pm0.27$ $2.01\pm0.17$ $0.34\pm0.10$ 27, 10 0.07, 0.11 this work
XO-1 $5754\pm42$ $4.61\pm0.05$ $1.07\pm0.09$ $-0.01\pm0.05$ 21, 9 0.04, 0.02 this work
XO-2 $5350\pm72$ $4.14\pm0.22$ $1.10\pm0.08$ $0.42\pm0.07$ 22, 9 0.05, 0.10 this work
CoRoT-Exo-1 $5950\pm150$ $4.25\pm0.30$   $-0.3\pm0.25^{a}$ Barge et al. (2008)
CoRoT-Exo-3 $6740\pm140$ $4.22\pm0.07$   $0.02\pm0.06^{f}$ Deleuil et al. (2008)
CoRoT-Exo-4 $6190\pm60$ $4.41\pm0.05$ $0.94\pm0.07$ $0.05\pm0.07^{a}$ Moutou et al. (2008)
GJ 436 $3350\pm300$ 5.0   $-0.02\pm0.20$e Maness et al. (2007); Bonfils et al. (2005)
HAT-P-3 $5185\pm46$ $4.61\pm0.05$   $0.27\pm0.04$ Torres et al. (2007)
HAT-P-5 $5960\pm100$ $4.368\pm0.028$   $0.24\pm0.15$ Bakos et al. (2007c)
HAT-P-8 $6200\pm80$ $4.15\pm0.03$   $0.01\pm0.08$ Latham et al. (2008)
HAT-P-9 $6350\pm150$ $\rm 4.29^{+0.03}_{-0.04}$   $0.12\pm0.20$ Shporer et al. (2009)  
HAT-P-11 $4780\pm50$ $4.59\pm0.03$   $0.31\pm0.05$ Bakos et al. (2009b)
OGLE2-TR-L9 $6933\pm58$ $4.47\pm0.13$   $-0.05\pm0.20$ Snellen et al. (2009)
WASP-1 $6110\pm45$ $4.28\pm0.15$   $0.26\pm0.03^{b}$ Stempels et al. (2007)  
WASP-2 $5200\pm200$ $4.3\pm0.3$   $0.1\pm0.2$ Cameron et al. (2007)
WASP-3 $6400\pm100$ $4.25\pm0.05$   $0.00\pm0.20^{a}$ Pollacco et al. (2008)
WASP-4 $5500\pm150$ $4.3\pm0.2$   $0.0\pm0.2^{a}$ Wilson et al. (2008)
WASP-5 $5700\pm150$ $4.3\pm0.2$   $0.0\pm0.2^{a}$ Anderson et al. (2008)
WASP-6 $5450\pm100$ $4.6\pm0.2$ $1.0\pm0.2$ $-0.20\pm0.09$ Gillon et al. (2009)
WASP-7 $6400\pm100$ $4.3\pm0.2$ $1.5\pm0.2$ $0.0\pm0.1$ Hellier et al. (2009)
WASP-10 $4675\pm100$ $4.40\pm0.20$   $0.03\pm0.20^{a}$ Christian et al. (2009)
WASP-11/HAT-P-10 $4980\pm60$ $4.54\pm0.03$   $0.13\pm0.08$ Bakos et al. (2009a)
WASP-12 $\rm 6300^{+200}_{-100}$ $4.38\pm0.10$   ${0.30^{\rm +0.05}_{-0.15}}^{a}$ Hebb et al. (2009)
WASP-13 $5826\pm100$ $4.04\pm0.2$   $0.0\pm0.2^{a}$ Skillen et al. (2009)
WASP-14 $6475\pm100$ $4.07\pm0.20$   $0.0\pm0.2^{a}$ Joshi et al. (2009)
WASP-15 $6300\pm100$ $4.35\pm0.15$ $1.4\pm0.1$ $-0.17\pm0.11$ West et al. (2009)
XO-3 $6429\pm100$ $4.244\pm0.041$   $-0.177\pm0.080^{c}$ Winn et al. (2008), updating Johns-Krull et al. (2008)
XO-4 $6397\pm70$ $4.18\pm0.07$   $-0.04\pm0.03^{d}$ McCullough et al. (2008)
XO-5 $5510\pm44$ $4.52\pm0.06$   $0.25\pm0.03$ Burke et al. (2008)
XO-5 $5370\pm70$ $4.31\pm0.03$   $0.05\pm0.06$ Pál et al. (2009)

The upper part of the table lists the parameters homogeneously derived using the method of Santos et al. (2004). The lower part contains data for all host stars of transiting planets not studied in this work but with stellar parameters and iron abundance or metallicity published elsewhere. a The cited value gives overall metallicity [M/H] rather than [Fe/H]. b They provide a value for overall metallicity of $0.23\pm0.08$. c They provide a value for overall metallicity of $-0.204\pm0.023$. d They provide a value for overall metallicity of $-0.02\pm0.05$. e The average of the values given by Bonfils et al. (2005) and Maness et al. (2007) is adopted here. f The abundance derived from Fe II lines is given. Deleuil et al. (2008) infer an overall metallicity of [M/H] $=-0.02\pm0.06$.


Source LaTeX | All tables | In the text

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