My triplet still get's some CA. If anyone is interested in the extreme details I'm willing to post more. The short version is that I've tried to do some spectroscopy with a grating, which revealed a "fishtail" in the violet/blue end of the spectrum that's produced by the stars.
What this translates to in imaging is violet/purple/ strong blue halo's around brighter stars. As an example I took RGB at 15sec exposures and put them together in PI. I only did an auto stretch (screen transform, histogram), star alignment, and finally channel combo to create the color image. Sure enough violet/blue halo's around the brighter stars.
I've contact the telescope manufacturer for assistance, and I'm waiting for a reply from their optical engineer.
However my fear at the moment is that replacement of the optics is what's going to end up being required, either by replacement of the lens cell, or by replacement of the whole OTA. Either way I'm looking at that much more "downtime". If I end up having to replace the OTA, I've been thinking about going to a newtonian, meaning a complete setup change.
I recently saw Adam's video on removal of scattered light, I wonder if something similar could be done for my blue frames?
Comments
To salvage something from your data you could try using a blue colour mask to select the halos and then replace with local background from a blurred copy, or perhaps using MT to shrink the halos on the blue channel. If most of the halos are on a dark sky background it's not too difficult to deal with, a bit more care is needed if they're in front of a galaxy or nebula.
Think of it as a challenge to get the best out of a data set with problems - that's what Adam's videos are all about!