| 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
HARPS RV measurements of K2-3.
 |
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% (20−30 days) and 0.0015% (8−10 days). The vertical lines indicate the period of Planets b, c, and d (from left to right). |
| Open with DEXTER | |
Model parameters: posterior mode and 68.3% credible intervals.
 |
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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