Usage
extrabol can be used directly from commandline:
extrabol 'filename.dat' ARGUMENTS
The following arguments are available:
--verbose
Increase output verbosity
-m MEAN, --mean MEAN
Use a supernova template as the mean function for the GP; Choose \'1a\',\'1bc\', \'2l\', \'2p\', or \'0\' (for no template)
Default = 0
-t, --show-template
Shows supernova template on plots as dotted lines
-d DIST, --dist DIST
Object luminosity distance in Mpc
-z REDSHIFT, --redshift REDSHIFT
Object redshift
If no argument is provided, redshift will be read from the input file
--dm DM
Object distance modulus
--plot BOOL
Output plots, Default is TRUE
--outdir OUTDIR
A file location for outputs to be written to
--ebv EBV
Milky Way extinction E(B-V) value, if known
If no argument is probided the extinction will be read from the input file
--hostebv HOSTEBV
Host extinction E(B-V)
-s START, --start START
Start time of analysis window relative to peak luminosity
Default = -50 days
-e END, --end END
End time of analysis window relative to peak luminosity
Default = 150 days
-snr SNR
Minimum signal to noise ratio for observations
Default = 4.0
-wc, --wvcorr
Use the redshift-corrected wavelength values for extinction calculations
-mc, --use-mcmc
Use a Markov Chain Monte Carlo to fit black bodies instead of curve_fit.
This provides better error estimates but takes much longer.
--T_max T_MAX
Modify the prior on temperature for blackbody fits by specifying a maximum temperature.
Default = 40,000K