Notes. The columns list: the ID code and evening date of the transit (or combined when the two transits were fitted together), the photometric channel (Bessel B or R), the number of data points analyzed, the RMS σ of the residuals from the best-fit model, the χ² and reduced χ² of the residuals, the linear LD coefficient u₁ (marked with † when it is input as a Gaussian prior around its theoretical value from Claret et al. 2012), the relative radius k of the best-fit model, and the relative radius k^′ after the correction for unocculted starspots has been applied (Ballerini et al. 2012; see Sect. 3.5 for details). The reported χ² and are evaluated from the nominal error bars once the bump-like feature has been removed (see Sect. 3.1). The RP error analysis is based on a residual-permutation algorithm (see Sect. 3.3 for details).