Display range is 0.8-1.2 for flats, 0.0-0.1 for deviations. The third image is the difference between the
canonical flat and the "super duper" grand canonical flat (computed from the average of periods 11-12) displayed at
a -0.03 to +0.03 stretch. Note that a separate "super duper" grand canonical flat was computed from periods 08-10
and subtracted from periods 01-10, to separate out the H behavior before and after the new array was put into the
telescope.
       
       
01 970000 970802 02a 970903 970922* 02b 970927 971026 02c 971027 971224 03 971225 980411 04 980412 980604 05 980605 980918 06 980919 981015 07 981016 981020 08 981021 981117 09a 981118 990129 09b 990130 990427 10 990428 990720 11a 990721 991030 11b 991031 000126 11c 000127 000321* 11d 000323 000901 12 000902 050000 * followed by nights w/o flats; will need to decide which canonical these nights go with. Original periods subdivided above: 02 970803 971224 09 981118 990427 11 990721 000901