deletions | additions       diff --git a/A_goal_of_this_work__.tex b/A_goal_of_this_work__.tex  index 110135b..65747a2 100644  --- a/A_goal_of_this_work__.tex  +++ b/A_goal_of_this_work__.tex 
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Specially, I'm trying to quantify the change in the SFR for different class of halo mass.  Has seen in the CODA simulation \cite{ocvirk_cosmic_2015}, I'm expecting a diminution of the instantaneous SFR in the less massive halo ($M<10^9M_{\odot}$).  I also see that the way energy is injected had a real impact on the results. I'll show that the choice of supernovae model is crucial, and the responce of the simulation can drastically change, while the total energy injected in conserved.  Furthermore I observe a dependency of the stellar mass resolution on how the reionization occur while the total number of emitted photons is conserved.  %I see that the way feedback is implemented has a big impact on the simulation response even if the total energy is the same.