Project goal: Determine best fit parameters for empirical Stellar-to-Halo Mass Relation (SHMR) model for dwarf galaxies in Bolshoi-Planck simulation, using MCMC techniques to fit to observed weak lensing and stellar mass function (SMF) data of dwarf galaxies from the COSMOS field catalog (Laigle et al. 2016).
Data: too large for GitHub. Actual data in lux:/data/groups/leauthaud/fardila/dwarf_lensingMCMC: most of the work is done here. This is where MCMCs were run to fit model parameters to data.notebooks: notebooks for initial tests in MCMC development.useful_halotools_scripts: python scripts for adding local particle and halo catalogs to halotools cache.