TOI-3288 b and TOI-4666 b: Two gas giants transiting low-mass stars characterised by NIRPS

Open Access

Fig. 3

Normalised CCF of TOI-3288. The upper panel shows the full CCF, while the lower panel shows the CCF with the BERV window $(\pm \frac{1}{2} F W H M)$ $Mathematical equation: $\[\left(\pm \frac{1}{2} \mathrm{FWHM}\right)\]$$ excluded. The Gaussian fit is indicated in orange (top) and green (bottom). The uncorrected RV is redshifted by ~300 m/s.

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