Shifted and combined CCFs for emission from Fe I. We detect the Fe I emission at a significance of 16.9σ, reproducing previous results. We were able to recover the signal near the expected planetary radial velocity. Yan et al. (2022b) obtained a 7.7σ detection, and Borsa et al. (2022) at 7.1σ with the Calar Alto 3.5m and the TNG 3.6m, respectively.