thanks, but what happens if you also add darks? last i remember the script will try to scale the darks for the flats... so if you have a 600s dark it's going to be scaling all the way down to 2s or so which seems dubious even for a "real" astro camera and certainly for a canon DSLR. of course if it does that it will also subtract the bias from the flat subs, so maybe everything is okay if the scaled dark turns out to be almost 0.
rob
Yes Rob, it will rescale the 600s dark down to 2s. I don't think this will work very well because there is a VERY non-linear transition in Canon DSLR's between exposures < 10 seconds and those > 10s. because of their interesting (and undocumented) internal processing. This processing is not "dark subtraction" ... it's something else. Looks like they may be messing with the dark pedestal?
What I find with my sensor running at ~-30c is that I have no hot/warm pixels and the dark current is so low that bias subtraction + flat division essentially leaves almost nothing (in both flats and lights) but shot noise.
I use a 200-frame master bias taken at -30c
If I try and use darks (either scaled or duration matched) the noise in the images increases significantly in both flats and lights. I've spent a long time analysing the noise figures for different combos of calibration!
If I was using a non-cooled Canon DSLR I would avoid dark scaling and use flat darks. I think other DSLR's (Nikon, Sony etc) would behave more like CCD's with regard to dark scaling...maybe?
I wish Canon would explain what they are doing on > 10s exposures - and it would be even better if it could be turned off!