KLEVER (Kmos LEnsed Velocity and Emission line Review) is an ESO Large Programme targeting around 200 galaxies at 1 < z < 2.5 with KMOS on the VLT. Galaxies are observed in all three primary near-IR bands (J, H, K; covering ~ 1.0 to 2.5 μm) in order to cover the full suite of rest-frame optical emission lines. This dataset will enable a detailed, spatially-resolved, investigation of the physical properties of the ISM at the peak epoch of cosmic star formation.

An example of an emission line and metallicity map for one KLEVER galaxy.

This ADS query gives an up-to-date list of all KLEVER-related papers.