Quote:
Originally Posted by sil
Something PI introduced "recently" (months ago, its been ages since I've used it) is a photometry colour correction (forget what its called but its standard in the package, Rick might chime in) that uses plate solving to look up reference data and make colour correction adjustment to get your star colours and nebulosity more accurate. Its an awesome tool and alone I have to redo my entire workflow as it shortcuts some steps I take to preserve colour changes while I process.
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It's called PhotometricColorCalibration. Lots of useful advice in this thread...
Cheers,
Rick.