Model evolution using energy distribution of the subhalo

astropradyumna / dwarf_formation

This is an attempt to form dwarf galaxies using a semi-analytic model based on Errani set of papers

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Open astropradyumna opened 5 months ago

astropradyumna commented 5 months ago

Errani models work better for energy distribution, try to use those

[x] Get the energy distribution for TNG subhalos
[ ] Come up with some way to save the best fit alpha and beta, to avoid recomputing
[ ] Errani models must be completely solvable for different $\alpha$ and $\beta$. Model this.
[ ] Check if the filter function can be fit by some other subhalos

astropradyumna commented 5 months ago

Unable to get good fits for the energy distribution probably because dN/deps blows up