If you have ever processed an astrophotographical image, you will have had to non-linearly stretch the image at some point, to make the darker parts with faint signal visible. Whether you used levels & curves, digital development, or some other tool, you will have noticed noise grain becoming visible quickly.
You may have also noticed that the noise grain always seems to be worse in the darker areas than the in brighter areas. The reason is simple; when you stretch the image to bring out the darker signal, you are also stretching the noise component of the signal along with it.
And that's just a simple stretch. Every pixel's noise component goes through many transformations and changes as you process your image. Once you get into the more esoteric and advanced operations such as local contrast enhancements or wavelet sharpening, noise levels get distorted in all sorts of different ways in all sorts of different places.
The result? In your final image, noise is worse in some areas, less in others. A one-noise-reduction-pass-fits-all no longer applies. Yet that's all that other software offers.
To establish this baseline, increase the 'Grain size' parameter until no noise grain of any size can be seen any longer.
No nonsense, affordable astro software that just works.
This way, nasty noise surprises when viewing the image at 100% are avoided.
And that's just what Tracking does for the deconvolution module.
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