wdinput.dat

# MCMC run parameters
fit      = 1      # actually fit (1), or just plot model as specified (0)

nburn    = 2000   # number of steps to use in burn-in phase
nprod    = 1000   # number of steps to use in production phase
nwalkers = 200    # must be even multiple of npars (npars = 4)

nthread  = 6      # number of CPU threads to use

scatter  = 0.10   # fractional scatter to add to starting ball of parameters

flat     = 0      # Is the chain file flattened, or 3D?
thin     = 1      # amount to thin MCMC chain by before calculating best fit


# All model parameters have both a starting value and a prior
# priors are specified by type, val1, val2
# type can be one of 'gauss', 'uniform' or 'log_uniform'
# if type = 'gauss', val1 and val2 represent mean and standard deviation of prior
# if type = 'uniform' or 'log_uniform', val1 and val2 represent the limits of prior


# # # # # # # # # # # # # # #
# Initial Model Parameters  #
# # # # # # # # # # # # # # #

# WD temp
# log g (model grid runs from 7 to 9.5, so within this as minimum)
teff  =   20000     uniform     5000     90000.0
logg  =   7.5       uniform     7.01     9.49

# Redenning E(B-V).
# If you don't know anything, should range from 0 to max galactic extinction
# at this position -> https://irsa.ipac.caltech.edu/applications/DUST/
ebv   =   0.01      uniform     0.00     0.0137

# Parallax prior and initial guess from Gaia
# -> http://gea.esac.esa.int/archive/
plax  =  2.4041     gauss     2.4041     0.1564


syserr = 0.03 # systematic error to add to all fluxes (in %)



# Name of chain file
chain = ../hierarchical_FinalFit/chain_prod.txt