A sample of ~1000 high-redshift (z ~ 0.3–1.7) star-forming galaxies has been observed with three-dimensional spectroscopy using the KMOS and MUSE spectrographs in order to explore the dynamical properties of galaxies across cosmic time. A summary of the survey is presented along with one set of results that explores the relationship between the angular momentum of the star-forming gas and galaxy morphology. This work expands previous angular momentum studies that mostly focused on local galaxies, to cover the past 10 billion years of cosmic time.