EDP Sciences
Free Access
Issue
A&A
Volume 581, September 2015
Article Number L7
Number of page(s) 6
Section Letters
DOI https://doi.org/10.1051/0004-6361/201525918
Published online 22 September 2015

Online material

Appendix A: Additional figures and tables

Table A.1

HARPS RV measurements of K2-3.

thumbnail Fig. A.1

Periodogram of HARPS RVs of K2-3. The horizontal lines correspond to 1, 2, and 3σ confidence intervals. The false alarm probabilities (FAP) of the main peaks are 0.044% (2030 days) and 0.0015% (810 days). The vertical lines indicate the period of Planets b, c, and d (from left to right).

Open with DEXTER

Table A.2

Model parameters: posterior mode and 68.3% credible intervals.

thumbnail Fig. A.2

As in Fig. 1, but for the K2 photometry of K2-3 (from top to bottom and left to right: planet b, planet c, and planet d). Each transit is centered relative to the linear ephemeris.

Open with DEXTER


© ESO, 2015

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