Hi Carles,
I did a quick process of the Ha part of the l-eNhance image and the NBAccent image. The Ha layer was processed in Mono with all the usual modules like Contrast, HDR, Sharp, SuperStructure (DimSmall) and Denoise. Stars were also deconvolved and shrinked.
The NBAccent image was only lightly processed since we only need the color information of it, right? Stars were neither deconvolved nor shrinked since my understanding of your explanation is that this isn't necessary. In SuperStructure I adjusted Saturation. The image was denoised in order to avoid chrominance noise.
Subsequently I loaded both images into layer and used 'Color of Foreground' for blending. This was the result:
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- Layer2.jpg (558.45 KiB) Viewed 2962 times
I guess we can agree that as you predicted there's more detail in the layered image and stars are much more reduced compared to the NBAccent image. I think that this could be compensated when stars are shrinked in the NBAccent image and when you go through all the modules like Contrast and HDR AFTER accenting the broadband image with the NB data which I haven't done here but in my original NBAccent image. Anyway, your prediction holds true and the result is consistent with your Bubble Nebula comparison.
I also had a closer look at nebula regions and some stars.
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- Layer1.jpg (280.85 KiB) Viewed 2962 times
In this magnification you can unfortunately see the oblong stars of my broadband image
Just ignore them. But what you can also see are some stars that have spikes in the NBAccent image but
not in the Ha image. As you would expect the nebula gets the blue spike colors although there are no spikes in the brightness/luminance layer. That's exactly what I meant with it being a problem when chrominance doesn't match luminance.
It becomes also obvious here:
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- Layer3.jpg (315.6 KiB) Viewed 2962 times
The central star is pretty small with no apparent halo in Ha but get's a strange coloring after layering. Looking at it you can sense that something's off here even if not pixel peeping and without knowing how the processing has been done. Some of the smaller stars appear with color halos since the broadband stars are bigger and the color of the complete star surface gets inherited to the luminance layer.
I don't say the method doesn't have its benefits. And maybe you can fix most or all of the issues. An obvious cure would be to shrink also the stars of the NBAccent image in the first place so you significantly reduce the halo effect. The spikes problem doesn't arise with refractors anyway.
But in my eyes the original NBAccent image is much more straight forward in terms of processing and it looks more natural. As I've said, the image was my first go at the data and almost certainly didn't take me an hour to get finished. I am a lazy processor so that approach appears more convenient to me. But if you are a tinkerer your method can certainly be put to good use.
Maybe I will give it another try on my next image. I was going for CTB-1, the Popped Ballon, and already acquired 11 hrs of duo NB data:
Can you see all those stars (deconvolved and shrinked) in the l-eNhance image? When I use a broadband image as base those stars will drive me nuts in processing. Also that thing is much fainter than the Wizard. You almost can't see anything in a single sub. So your layering might be much more straight forward than the conventional NBAccent.
Regards
Stefan