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I'm working with Emma, an AMR cosmological code with fully coupled radiative hydrodynamics, in which one I've implement a star formation recipe and different types of supernovae feedback.  I'll show that with a wildly use star formation recipe, based on a simple density criterion, we fit the observed cosmic Star Formation History on redshift going from 10 to 5.  I'll then use Starburst99, a stellar population model, to constrain some free parameters of my model like the lifetime or the intensity of sources.  I'll also present how I've implement thermal and kinetic supernovae feedback, and the way theses feedback impact the Star Formation Rate during coupled runs.