Binarity of transit host stars - Implications for planetary parameters

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Table 4:

Individual binary component parameters.
$\begin{displaymath}{ \begin{tabular}{lccr@{~$\pm$~}lccr@{~$\pm$~}lr@{~$\pm$~}lr@... ...&50 & \multicolumn{2}{c}{}& \\ [0.5ex] \hline \end{tabular}} \end{displaymath}$ ^a The stellar secondary is referred to as ``/C'' in order to avoid confusion with the notation of the planetary companion, which is referred to as an appendix ``b'' to the host star's name in many publications. ^b Uncertainties of apparent magnitudes are estimated to be $\delta\rm {mag}=0.10$ (see Sect. 4.1). ^c Separation and period estimates use distances from Table 2. ^d Periods are order-of-magnitude estimations and hence do not include an uncertainty estimation.

Source LaTeX | All tables | In the text

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