TODO list

find a good estimator for the error of the fit (chi squared? Something else?)
find a good fit for the correlation coefficient for all redshift pairs
check dependence of fit on initial seed (optional, probably minimal as we're interested mostly in small scales)
check dependence of fit on cosmological parameters
check if correlation coefficient can be computed with COFFE in reasonable time (optional)
verify that cutoff k ~ 7 h/Mpc is sufficient (baryonic physics?)
check for convergence w.r.t. different simulation parameters
check CLASS HALOFIT and HMCode for accuracy and speed as comparison for nonlinear power spectra

Name		Name	Last commit message	Last commit date
Latest commit History 10 Commits
daint_2048		daint_2048
daint_2048_smallbox		daint_2048_smallbox
example_plots		example_plots
README.md		README.md
process.py		process.py

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