| Issue |
A&A
Volume 582, October 2015
|
|
|---|---|---|
| Article Number | A54 | |
| Number of page(s) | 14 | |
| Section | Planets and planetary systems | |
| DOI | https://doi.org/10.1051/0004-6361/201526196 | |
| Published online | 05 October 2015 | |
Online material
Appendix A
Radial velocities measured with CRIRES.
 |
Fig. A.1
Median-combined spectra from detector 1 for all observed targets, shifted by +0.5 in ascending order starting from K4 III giants at the bottom to earlier spectral type stars toward the top. Telluric lines were removed. Obviously late G and early K giants have a smaller number of deep stellar lines in this wavelength region than later K giants. |
| Open with DEXTER | |
 |
Fig. A.2
Same as Fig. A.1, except for detector 4. Detector 4 has in general lower S/N when compared to detector 1. |
| Open with DEXTER | |
© ESO, 2015
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