Title: SINFONI-HiZELS: Tracing the formation and evolution of star-forming galaxies across 
cosmic time

Abstract:
There is copelling evidence that in ''normal galaxies'' at z ~ 1 - 3, the mechanism that dominates 
the accretion of gas (reservoir for star-formation) is via cold streams from the inter-galatic 
medium, this means most of the star formation is probably driven by internal dynamical 
processes. On the other hand, the present capabilities of IFU spectroscopy are now delireving 
resolved imaging of z ~ 2-3 galaxies on ~ kpc scales (~0.1”), so we can measure the internal 
properties of high-z galaxies. We present the first results obtained from adaptive-optics assisted 
IFU spectroscopy of 18 H-alpha emitters (from HiZELS) with SINFONI on the VLT.