Volume 582, October 2015
|Number of page(s)
|Planets and planetary systems
|01 October 2015
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 .
|Open with DEXTER
Priors used in the PASTIS analyses.
Posterior distributions of the PASTIS analyses.
© ESO, 2015
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