[chains]
# Total number of samples: n_walkers * (n_steps - n_burn_in)
#
# Number of chains.
n_walkers=100
# Number of initial steps thrown away for each chain.
n_burn_in=2000
# Number of steps taken by each chain.
n_steps=1000


[tables]
# Catalog containing input magnitudes for the fitting.
# May be:
#    a. FITS file obtained by VO service.
#    b. HDF5 file imported from deepdish legacy catalog.
#    c. ASCII tables.
mags_catalog=data/jplus-dr3/input/jplus-dr3_psfcor_zsdss.fits


# Use spectroscopic redshifts for the fitting (if column z_spec is available).
use_spec_z=False

# Filter table
filters_table=data/jplus-dr3/filter.fits

# Directory containing the filter curves.
# These must be in increasing wavelength.
filters_dir=data/JPLUS_filter_curves

# Filter filename pattern, to be interpolated with filter name.
filters_pattern=JPLUS_%s.tab

# Output catalog.
#chains_db=data/output_AEGIS201910/output_chains_AEGIS_idr201910_mag_auto_jpas_r2270_Avmax2.hdf5

chains_db=data/jplus/output/jplus-dr3_m2275_auto_zml_delayed.hdf5

# Base HDF5 file.
base_file=data/Base.cb17.chab.7met.All.hdf5

# Base name in HDF5 file.
base_path=cb17

# debug plot output dir
plots_dir=data/jplus-dr3/plots

[taylor_mat]
# Taylor matrix, created by matrix_ssp.py
#taylor_file=data/m_a_JPAS.cb17.chab.7met_z1.hdf5
taylor_file=data/jplus-dr3/m_a_jplus-dr3.cb17.chab.7met_z1_fixed_H068.hdf5

# Redshift sampling
z_ini=0.001
z_fin=1.
z_delta=0.001

# Order of Taylor expansion
n=3

[fitting]
# Parametric model of SFH.
# Models available: exp, delayed_exp, sandage, square, lognormal
# t0 range, in units of the age of universe (taken from z).

#param_model=delayed_exp
param_model=delayed_exp

#t0_min_scale=0.01
#t0_max_scale=0.99

# Tau range, in units of t0.
#tau_min_scale=0.001
#tau_max_scale=2


# Prior mode: uniform, scaled
prior_mode=uniform

# t0 range, in units of the age of universe (taken from z).
#t0_min_scale=0.01
t0_min_scale=0.1
t0_max_scale=0.99

# Tau range, in Gyr.
# Used if prior mode is "uniform".
tau_min=0.1
tau_max=10.0

# Tau range, in units of t0.
# Used if prior mode is "scaled".
tau_min_scale=0.01
tau_max_scale=1.0

# Minimun fraction of unflagged/unmasked filters required.
min_filter_fraction=0.5 

# Reddening range
AV_min=0
#AV_max=1
AV_max=2


# Wavelength of base normalization window.
# Used when calculating light weighted ages.
lambda_norm=5635.0

# Mask (ignore) filters when fitting (1 = mask).
# This is a list the same length as the number of filters.
filter_mask=[0,0,0,0,0,0,0,0,0,0,0,0]

# Consider narrow the filters with width smaller than this value.
narrow_width=200.0

# List of emission lines to mask when fitting.
# To disable, use an empty list:
#em_lines=[]
#em_lines=[3727.0, 4861.0, 4959.0, 5007.0, 6548.0, 6563.0, 6583.0, 6717.0, 6732.0]
em_lines=[]

allow_blended_mags=True

[cosmology]
H0=68.0
omega0=0.310

[grid]
remote_data=http://minerva.ufsc.br/~andre/JPLUS_data