Sketchs of the different scenarios considered for the PASTIS validation of the two planets in the K2-19 system. The sizes are not proportional to their real values but note the relative size of the orbits between the 8-d and 12-d signals. Note also the orbit of the contaminant system in scenarios to , which marks the difference between these and the unbound scenarios to .
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Priors used in the PASTIS analyses.
Posterior distributions of the PASTIS analyses.
© ESO, 2015