Open Access

Fig. 1


Automatically created post-vetting data for Wendelstein-1b. Top: stellar parameter fits with the results from SED fitting (yellow) and spectroscopy (green) with an underlying χ2 contour plot of log g against effective temperature based on SED fitting. Bottom: folded light curve with the best-fitting model (blue line) and data from Pan-Planets (black circles) and WWFI of the 2 m Wendelstein telescope (red diamonds). Note: the internal convention of Pan-Planets was to place the primary transit at phase 0.5; the y-axis of the residual frame was by default zoomed out to better assess the goodness of the fit.

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