Full reference data set

To recap various formal and non-formal conversations, here is the data set we would like taken after each instrument reconfiguration, cool down, or disassembly. And once a month in any case.

In order:

• 15 biases
• 15 300s darks
• dithered flats, currently 20 roughly 0.3 pixel steps on each side of nominal. Three exposures at each position.
• 5 flats at nominal position.
• 5 Ne arcs, with peaks at 40k or so
• 5 HgAr arcs peaks at 40k or so
• any other arc lamps, 5 exposures with peaks at 40k