Free Access
Volume 575, March 2015
Article Number A71
Number of page(s) 15
Section Planets and planetary systems
Published online 25 February 2015

Online material

thumbnail Fig. 11

Third-body mass allowed by the RV drift for a given period assuming circular orbits for KOI-206 (left) and KOI-680 (right). The median of the distribution is represented by a solid line, and the 1, 2, and 3σ confidence intervals are represented with three different gray levels. The dotted lines separate the planetary, brown dwarf, and star regimes.

Open with DEXTER

thumbnail Fig. 12

Two-parameter joint posterior distributions of the MCMC jump parameters of the fit with stellar models of KOI-206. The 39.3%, 86.5%, and 98.9% joint confidence regions are denoted by three different gray levels. The histogram of each parameter is shown at the top of each column, except for the parameter on the last line that is shown at the end of the line.

Open with DEXTER

thumbnail Fig. 13

Same as Fig. 12 but for KOI-614.

Open with DEXTER

thumbnail Fig. 14

Same as Fig. 12 but for KOI-680.

Open with DEXTER

© ESO, 2015

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