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

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Table 1:

Characteristics of transiting planets included in this study.
$\begin{displaymath}\begin{tabular}{>{$}l<{$}>{$}r<{$}>{$}r<{$}>{$}r<{$}>{$}r<{$}... ...\_3} & {>}82.7 & 0.051 & [Udalski07] \\ \hline \end{tabular}\end{displaymath}$ Underscores indicate uncertainties on last printed digits. Bracket = announcement paper. No bracket = reference from which most parameters have been chosen from. *=also in Torres et al. (2008). $M_{\rm Jup}=1.8986112\times 10^{30}~$ g is the mass of Jupiter. $R_{\rm Jup}=71,492~$ km is Jupiter's equatorial radius. References: Winn et al. (2005); Charbonneau et al. (2006); Torres et al. (2004,2007); Winn et al. (2007a); Minniti et al. (2007); Winn et al. (2007c); Mandushev et al. (2007); Burke et al. (2007); Shporer et al. (2007); Gillon et al. (2006); Pont et al. (2004); Gillon et al. (2007); Kovács et al. (2007); Sozzetti et al. (2004); Winn et al. (2007b); Alonso et al. (2004); Bouchy 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); Holman et al. (2006); Bouchy et al. (2005); Charbonneau et al. (2000); Knutson et al. (2007); Pont et al. (2008). The table is derived from Frederic Pont's web site: http://www.inscience.ch/transits/. $^{\star \star}$ HD147056 is also called HAT-P-2.

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