KLEVER (Kmos LEnsed Velocity and Emission line Review) is an ESO Large Program exploiting the KMOS multi-IFU near-IR spectrograph at the Very Large Telescope, to obtain 3D spatially resolved spectroscopy of a sample of about 200 galaxies in the redshift range z~1-2.5, in all three primary near-IR bands (J, H, K). The main goals are to characterize the evolution of the physical properties and chemical enrichment of galaxies across the cosmic epochs.
https://www.kicc.cam.ac.uk/projects/klever
