Sample plist output

##
## SPECDETECT -- locate peaks in 1-D grating data
## 
input_data_file =                  input data file [root.dat]
#
# Data columns are: col1=position, col2=optional bin width
# if bin width present: col3=counts or flux, col4=counts_err or flux_err
# if bin width not present: col2=counts or flux, col3=counts_err or flux_err
#     
num_cols_in_data = 3                number of columns in input data file
flux_corrected = no               Is the input file flux corrected?
output_peaks_file = .                output file name [root.peaks]
output_continuum_file = .                output continuum file name [root_cont.dat]
data_minus_cont_file = .                output (data-continuum) file name [root_nocont.dat]
thresh_emission = 4                emission line detect threshold = (thresh_emission * uncertainty)
       grating = HEG              Grating associated with the input data
#
# If entering an input continuum spectrum, all 4 columns must be present:
# col1=lambda, col2=bin width, col3=counts or flux, col3=counts_err or flux_err
#
(input_continuum_file = NONE)            optional input continuum file name [root_cont.dat]
(thresh_absoption = 2)               absorption line detect threshold = (thresh_absorption * uncertainty)
#
# The methods for calculating the continuum are:
#	median  -> running median using median_n_bins, with step size of 1 bin
#	tmedian -> running truncated median using median_n_bins, ""
#	spline3 -> cubic smoothing spline
# If using median or truncated median, must set the median_n_bins parameter
#
(continuum_method = median)          Continuum calculation method
(median_n_bins = 50)              Number of bins for median of continuum calc - EVEN number
  (cont_offset = 1)               Offset from line center to sample continuum [LSF width]
#
# The of head and tail of the non cubic spline continuum calculations need to
# be determined by the user.  The head and tail sections are equivalent to
# median_n_bins/2 on each end of the spectrum.  Currently, the possible 
# values for those sections are:
#	default     -> sets the head and tail to = 0 counts
#	values      -> sets the head and tail to user values; values are set
#                      in the following paramerters called "head_value" and
#	               "tail_value"
#	extrapolate -> uses extrapolation of the neighbors to cal head/tail
#	copy        -> uses a copy of the neighbors data values to get the extra
#	               points in order to perform median/tmedian calculations 
#
(head_tail_cont_method = default)         Head and tail t/median continuum calc
#
# If head_tail_cont_method=values, the values must be set here, using
# the parameters "head_value" and "tail_value".
#
   (head_value = 0)               If head_tail_cont_method=values, set short wavelength (left) end
   (tail_value = 0)               If head_tail_cont_method=values, set long wavelength (right) end
#
# If using the truncated median parameter, set the low and high cut offs.
# The (high_tmedian + low_tmedian) cut off, must be less than 1.
#
  (low_tmedian = 0.2)             For truncated median, reject bin values <= (low_tmedian * median)
 (high_tmedian = 0)               For truncated median, reject bins values >= (high_tmedian * median)
      (clobber = yes)             OK to overwrite existing output files?
        (debug = 1)               debug level (0 = no debug)
         (mode = ql)