Hello dear Astropeeps,
I am still rather new to the SHO palette with a mono-camera and I just completed my third image on the North American Nebula and never collected as much data for an image as of now. I love to see the separation of gases and how the interaction of different colors create different new combinations such as the SII and OIII interactions create magenta patches.
I also take great care to calibrate and balance the intensity between the channels and as a result there are also parts of the image that are green from the H-Alpha. I intentionally left those areas untouched, because
a.) I like how it looks like (we collect a whole third channel to introduce more color, why get rid of) and
b.) it feels unscientifical to run SCNR to get rid of it.
My question to you is: What is your approach with the SHO palette? Do you leave the green in or not?
I am also more than open to hear (constructive) criticism towards my processing and hear your opinion on my latest image.
CS,
David
I am still rather new to the SHO palette with a mono-camera and I just completed my third image on the North American Nebula and never collected as much data for an image as of now. I love to see the separation of gases and how the interaction of different colors create different new combinations such as the SII and OIII interactions create magenta patches.
I also take great care to calibrate and balance the intensity between the channels and as a result there are also parts of the image that are green from the H-Alpha. I intentionally left those areas untouched, because
a.) I like how it looks like (we collect a whole third channel to introduce more color, why get rid of) and
b.) it feels unscientifical to run SCNR to get rid of it.
My question to you is: What is your approach with the SHO palette? Do you leave the green in or not?
I am also more than open to hear (constructive) criticism towards my processing and hear your opinion on my latest image.
CS,
David