Changes
/* For IRAF users */
== For IRAF users ==
Since most observers seem to have their own scripts from the old version of the spectrograph, the easiest way to reduce the data is to use the QL wavelength -calibrated outputs as a reference for an IRAF reduction of the raw data.
This assumes familiarity with reducing longslit data in IRAF. Phil Massey's guide is an excellent reference: http://iraf.noao.edu/iraf/ftp/iraf/docs/spect.ps.Z
