Hi everyone,
I am working on a narrowband project and the best stretching method for obtaining nebular detail and equilibrium (O3 is really faint) in this cas was Masked Stretch. However the bigger stars in the image have completely saturated circular white core with a net separation from the rest of the star (similar to the deconvolution artefact when the stars are not masked). Is this a known artefact of masked stretch on big stars and are there any setting for obtaining a more gradual tapering of the signal from the center of the star?
Thanx.
Bogdan