Rebecca works on the evolution of high-redshift galaxies (z >= 4). Her previous experience is in using ground-based optical and near-infrared data to search for luminous sources up to z = 10 and to compute their evolving luminosity functions. She is co-lead of the Photo-z and SED fitting group within the Galaxies group, where she works on simulating high-z galaxy populations that will be found from combing Rubin with Euclid data
