Hi Adam,
I watched your 10 Part WBPP videos on Youtube before deciding to purchase Fundamentals. Very clear, and with reasons behind the usage. Part 9 was very helpful. Previously I used a CCD camera had been using more the CCD workflow for my new CMOS cooled camera. Happily I discarded all my biases and made some flat darks! No more optimizing with super long exposure darks! Everything matching is best.
I know many things in image processing are not clearly right or wrong, and I really appreciate what I learned especially in the latter parts of OGC300 Workflow example. In this example the data provided to you had bias frames and no flat darks. You had darks that did not match the lights. This really surprised me after watching WBPP Part 9 for CMOS cameras.
Using bias frames as flat darks (and forcing the times to match), and forcing the darks times to match the lights seemed wrong. Thinking back the provided flats for OGC300 were several different exposures, I think difficult to provide matching flat darks.
The OGC300 example bends the logic of WBPP where Calibrate with Flat Darks checkbox means they time-match, and then you show how the bias can be a Flat Dark. With the data given, you certainly processed the calibration as best possible with the data given, and in the end show show an image that is very nice. This should give imagers without the greatest calibration data confidence how to process it.
For me, I will be making matching Flat Darks with light panel Flats, and matching Dark exposure times with Lights! Now I really need to work on post calibration!
Thanks,
Roger
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