There were no calibration spectra taken this run, so the quartz lamps were taken from the observer in the A half of the night (NM08, Hami).  Also, there were two standard star spectra, but they are not nodded, therefore I could not use them to reduce.  I used a standard star from one of the previous runs (Jan 15, 2009) that was at an airmass of (1.59-1.68).