Interpreting the yield of transit surveys: are there groups in the known transiting planets population?

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Table 2:

Characteristics of stars hosting the transiting planets included in this study
$\begin{displaymath}\begin{tabular}{>{$}l<{$}>{$}r<{$}>{$}r<{$}>{$}r<{$}>{$}r<{$}... ... \pm{91} & 0.11 \pm{0.10} & Udalski07 \\ \hline \end{tabular}\end{displaymath}$ Underscores indicate uncertainties on last printed digits. *=also in Torres et al. (2008). References: Winn et al. (2005,2007a); Torres et al. (2007,2004); Charbonneau et al. (2006); Minniti et al. (2007); Winn et al. (2007c); Shporer et al. (2007); Burke et al. (2007); Mandushev et al. (2007); Bouchy et al. (2008); Gillon et al. (2006); Pont et al. (2004); Gillon et al. (2007); Kovács et al. (2007); Sozzetti et al. (2004); Winn et al. (2007b); Bouchy et al. (2004); Alonso et al. (2004); O'Donovan et al. (2006); Sato et al. (2005); Collier Cameron et al. (2006); O'Donovan et al. (2007); Konacki et al. (2003); Bakos et al. (2007); Knutson et al. (2007); Charbonneau et al. (2000); Bouchy et al. (2005); Holman et al. (2006); Pont et al. (2008); The discovery Papers are in brackets. The table is taken from Pont's site: http://www.inscience.ch/transits/.

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