EDP Sciences
Free Access
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

Table A.1

Radial velocities measured with CRIRES.

thumbnail 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

thumbnail 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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