Fig. 7

Orbital scheme the solution found for the orbit of the planet Kepler-447b (red filled circle). Left panel: pole-on view of the orbit (separation from the star in units of the stellar radius). We show 500 orbits by bootstrapping the parameters inside their uncertainty limits. Right panel: face on view of the orbit as projected in the sky (separation from the star in units of the stellar radius). We have marked the path of the planet between the dotted lines. The gray solid lines represent 500 orbits by bootstrapping the impact parameter. We can see that the transit is always grazing independently of the parameters taken inside the uncertainty limits.
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