deletions | additions       diff --git a/I_ll_show_that_with__.tex b/I_ll_show_that_with__.tex  index a406075..86fdb71 100644  --- a/I_ll_show_that_with__.tex  +++ b/I_ll_show_that_with__.tex 
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I'll %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 %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 %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. I'll %I'll  finally show that with a correct Star Formation History and a correct emissivity model we obtain a reionization history and a halo luminosity function in accordance with the observations. Finally, %Finally,  based on a fiducial run, I'll present a set of run with different feedback parameters and I'll show that the way supernovae energy is injected is really crucial in term of star formation response.