Syntax: makeepipe  ( all | (file with list of files) )
    [ step={1,2,3,4,5,6} ]  [ skip={1,2,3,4,5,6} ]
    [ raw= ]  [ bias= ]  [ -noobject ]  [ -norename ]
    [ echtol= ]  [ xdtol= ]  [slittol=]  [fttol=]  [-verbose]
    [ eperdn= ]  [ ronoise= ]  [ sat= ]  [ pf= ]
    [ imagelist=]  [scriptname=]  [observer=]  [prefix=]
    [ -update ]  [ -cycle sleep= [ stopin= | stopat= ] ]
    [ lpr= ]  [-lesspr]  [ -nomedian ]  [ -log ]
    [ -addarc ]
  
    [ -help (see complete description of options) ]
    [ -options (see complete description of options) ]
  
    Reduces HIRES FITS files.  Makes observations listing,
    creates bias frame, groups and averages flat fields,
    sets up and  executes script to run "makee" on objects.
  
    The first parameter is required.  If "all" is given then
    all the ".fits" files in the raw image directory are used.
    Alternatively you can specify a file containing a list of
    FITS files in the raw image directory, or if step#1 is
    excluded then the filenames are read from "image.list".
  
    The two files "exclude.list" and "exclude.redux" can be
    used to list files to be excluded from the listing and/or
    from the reductions.
  
 Options:
   step=    : Specify one or more steps to be executed:
                 (default: execute all steps)
      (1) = Create listing file "image.list".
      (2) = Find e-/DN and readout noise using darks, flats.
      (3) = Create BIAS.fits image file.
      (4) = Average flat field images.
      (5) = Write "makee.script" script file.
      (6) = Execute "makee.script" script file.
  
  skip=     : Skip one of more steps.
  raw=      : Directory name for raw HIRES image files
                 (default= current directory.)
  bias=     : Name of bias file (for makee) (if specified,
                  skip step #3.)
 imagelist= : File with "makeepipe-style" listing of HIRES FITS
              files to reduce (if used, step #1 is skipped).
  -noobject : Do not change object name (using .list file)
  -norename : Do not rename lamp files: [lamp/filter]
  -nomedian : Do not calculate medians for listing file.
  -log      : Send "makee" output to log files.
  -addarc   : Use additional arclamps (if available.)
  -update   : Extract only new objects (i.e. only extract
                  objects without a Flux-*.fits file.)
  -cycle    : Cycle program in loop (implies "-update").
 stopin=h   : Stop cycling in "h" hours (default=12).
 stopat=HH:MM : Stop cycling at "HH:MM" (HST).
 sleep=     : Sleep time between cycles in seconds (def=180).
 scriptname=: Filename for the makee script.
  observer= : Change all OBSERVER cards to this string.
   prefix=  : Prefix to RAW FITS file names, e.g. "hires".
  lpr=      : Send makee output to this printer.
  -lesspr   : Send less output to printer (just Flux*.fits).
  pf=       : Use this parameter file (default: makee.param)
  echtol=   : Echelle angle tolerance (default= 0.001).
                (To qualify as the same setup.)
  xdtol=    : Cross disperser angle tolerance (default=0.0016).
  slittol=  : Slit width tolerance (default=0.2).
  fttol=    : Flat averaging delta-time tolerance in minutes.
                (acceptable time seperation) (default=60.)
  eperdn=   : Electrons per digital number (for makee).
  ronoise=  : Readout noise in electrons (for makee).
                 (if eperdn= or ronoise= used, skip step#2.)
  sat=      : Saturation level in digital number.
                 (default=  64000.)