
31-12-2013, 04:55 PM
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Registered User
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Join Date: Jul 2013
Location: Cecil Plains QLD
Posts: 1,228
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Quote:
Originally Posted by RickS
I have spent a fair amount of time experimenting with methods for doing this in PixInsight. Similar techniques can probably be used in other image processing packages...
The best way I have found so far is to decompose the NB and RGB images into CIE L*a*b* channels. A star mask is used to protect everything except the stars in the NB a* and b* channels. Blend the RGB a* data into the NB a* and the RGB b* into the NB b*. Then recombine the NB L* with the modified NB a* and b* and voila! This works well because it only changes the colour of the stars and leaves the stellar profile (Lightness channel) unchanged.
Cheers,
Rick.
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Thanks for the info Rick  great to have on hand.
Jo
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