Quote:
Originally Posted by irwjager
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Well Ivo after having a read about what your software does I think I understand what is going on. I am very impressed.
The difficult part is to come to terms with the 'look' of the image. I am sure it is because I/we am/are not used to seeing the real information that is normally hidden. It is akin to seeing everybody without their clothes in public!
There is a Hubble Palette colour 3nm NB image further back in this thread at post 20. Could I impose on you to give that a shot as well. I would be very interested what you can do to minimise gradients, the curse of the widefield imager.
You are of course welcome to use my data as examples etc.
Bert