deletions | additions       diff --git a/I_m_working_with_Emma__.tex b/I_m_working_with_Emma__.tex  index 36a2deb..cf14f2b 100644  --- a/I_m_working_with_Emma__.tex  +++ b/I_m_working_with_Emma__.tex 
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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.  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.  Based 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.