Christophe Lovis' research focuses on the multiple applications of high-resolution spectroscopy to the field of exoplanets. He is a specialist of high-precision radial velocity measurements for the detection of exoplanets, and has contributed to the development of several state-of-the-art spectrographs, e.g. HARPS, HARPS-N, and ESPRESSO. In particular, Christophe Lovis has been the main developer of the data reduction pipelines for these instruments. He contributed to the discovery and characterization of many low-mass planets in the super-Earth to sub-Neptune regime. Prof. Lovis is currently leading the transit follow-up working group within the ESPRESSO Consortium.