I saw that on the cores. I wonder what's up. The reference images I looked at were, of course, significantly longer length, perhaps thus spreading those bright galaxy cores over more pixels and better resolving. At shorter length, they may really be concentrated into just a few pixels?
Anyway I tried to teach myself PI CFAD today.
Ultimately I did end up with a result of sorts. He he. Boy PI sure needs a Guy to write up user notes and special techniques for them. I fear that all the number crunching my CPU did on subframe weighting and local normalization went for naught, as I don't think I properly loaded and enabled that when I got over to drizzle integration. Bonkers. I'll have to retry later.
That said, even botched up by my errors, the output is way better than DSS CFAD. In DSS of course you just check a box. PI requires jumping through all sorts of hoops. But perhaps worth it.
I had no strange color errors, and barely any background "gridding." The only time I saw even a hint of that was via ST's scaling emulation, and even then only at something odd like 48% zoom. All other scales looked great.
I still binned 50% though. SVD just did not like full resolution, and any non-apod-outlined star (there were a lot of them too) had gnarly black eye ringing that would not correct. But at 50% I had beautiful green core stars all over the place for sampling.
That was with the HOO (L-eNhance), so I went ahead and also did CFAD on my discrete SII filter data. This was all back in Feb 2022 when I was experimenting with duoband + SII acquisition with the D5300.
I don't know PI well enough to find my duoband reference and stack the SII to it, so I just star aligned afterwards. Then I extracted the R from both files to get Ha and SII, and then used the duoband G for my OIII, ditching the B.
Used ST compose and weighted the channels according to probable relative SNR after running the PI noise estimator on the files.
I think it came out okay perhaps. Especially for this way old DSLR data and that I was using the MPCC at the time which blurs up all the data in the center. I think I'm fairly impressed with PI CFAD. Imagine if I had done it correctly!
I do have hot pixels all over, since I had no darks only bias, and also didn't set up rejection parameters so I think this is straight averaging. Also got me a little sat trail due to that also.
February 2022 Rosette in "true" OSC SHO, now with PI CFA Drizzle and ST 1.9 beta:
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- Rosette Feb 2022 PI CFAD OSC-SHO ST9 1B 1600.jpg (615.78 KiB) Viewed 26187 times