param_raw.yml

# Except for the output and filename, what is left out is read from the defaults.yml file.
# Information about the data file
FileName:       'data/obs-18-11-2016/B0329 54.2016.11.18.1038.5min.dat'
RawData:        true
FileFormat:     'raw'              # raw, fits, or fil (future...). Optional, overwrite automatic determination from extension
ObsMetaData:                           # Only necessary if RawData is true
  ObsDate:      '2016-11-18T10:18:00.00(UTC)'        # optional, only for raw data. Format readable by astropy.time.Time (see )
  PulsarName:   'B0329+54'          # optional only for raw data
  MixFreq:      405                 # optional only for raw data, in MHz.

# Folding parameters
Folding:
  nbins:          500           # Number of bins for folding 
  nbinsdedisp:    500           # Number of bins for dedispersed profile

# Output parameters
Output:
  OutputDir:      './output'    # Will overwrite any old files without warning.
  ConvertRaw:     true         # if raw convert to fits and write to OutputDir
  SavePlots:      true          # Saves all relevant plots in OutputDir
  
# If not wanted, you can just set ChiFit to false, and nothing will be done:
# ChiFit: false

# Chifit parameters
ChiFit:
   Ntries:       1000           # How many periods to calculate the average over
   nbins_time:   1000           # Amount of time bins to be used for calculating chisquared
   nbins_freq:   1000           # Amount of freq  bins to be used for calculating chisquared
   trywidth:     1e-3           # Time width of the period tries: (1-width)P_lit<P_try<(1+width)P_lit
   FitFunc:      'Lorentzian'   # Fit function to fit to the chisq as function of trial period. If left empty, will try all and prompt the user. 
 

# RFI removal scheme
GrasMaaier:
  STDCut:          5         # from which amount of STD do we cut
  FilterType:      'pyramid' # type of filter, 'pyramid' or 'tophat' possible.
  FilterWindow:    100001    # Number of data points to be used for the smoothed function.