The October 2000 version of makee includes a few significant changes and
additional features:

New for October 2000:
  ) Reduces ESI echellette data (1x1) as well as HIRES data (1x1,1x2).
  ) Runs on PC/Linux (gcc,g77) systems as well as Sun/Solaris.
  ) Reduces single amp. and double amp readout data for ESI and HIRES.
  ) Created "esipipe" program for easier ESI run reductions.
  ) Added "oko=" option.
  ) Added "uop=" option.
  ) New program "cpgim"-- a simple interactive PGPLOT image display program.
  ) "xplot" can now overplot multiple 2-D spectra.

New for March 2000:
  ) "Y2K" bug fix-- prevents possible heliocentric velocity error.
  ) "bracketting" arc lamps: If you have an arclamp taken before and after 
       your object, makee will generate an "averaged" wavelength scale.  
       This is important for night-sky-line-deficent UV cross disperser 
       observations.

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