The KMOS Lens Amplified Spectroscopic Survey (KLASS) kinematics and clumpiness of low mass galaxies at cosmic noon
We present results from the KMOS Lens Amplified Spectroscopic Survey (KLASS) an ESO Very Large Telescope (VLT) large program using gravitational lensing to study the spatially resolved kinematics of 44 star forming galaxies at 0.6 1) we find a weak increase or flat trend. We investigate the relation between the rest frame UV clumpiness of galaxies and their global kinematic properties. We find no clear trend between the clumpiness and the velocity dispersion and \upsilon_{rot}\sigma_0$ This could suggest that the kinematic properties of galaxies evolve after the clumps formed in the galaxy disk or that the clumps can form in different physical conditions.