
I am a bit unclear on the instrumental response part, not how to perform it, but the order of operations. For example: (1) pick an A0 star 4-6 mag to determine instrumental response from the Miles list, calibrate it and use it to determine response. (2) Then image another Miles standard in the same area for practice and see how I do.
This seems clear from Christian's Lisa tutorial. Now, if I go to another part of the sky, will I have to determine instrument response again? I would guess I do, since the response is "in the atmosphere." Rather like differential photometry rather than all sky photometry?
Looking forward to using my ALPY,
Ed