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I'm \begin{itemize}  \item   \end{itemize}I'm  working with Emma, \cite{aubert_emma:_2015} Emma \cite{aubert_emma:_2015},  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 widely 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.