Open Access

Fig. 10

image

Total cross correlation signal from single-night observations of 51 Pegasi with VLT/CRIRES, shown as a function of planet rest-frame velocity (V rest) and maximum orbital radial velocity KP. Left column: analysis without any removal of the stellar spectrum, right column: analysis after removing the stellar spectrum with the tools described in this work. The expected contamination of stellar lines (mostly CO) is marked with dashed white lines. This figure should be compared with Fig. 2 of Brogi et al. (2013).

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