Hi All,
Can someone help me to understand the basics of how channel extraction and mapping in Pixinsight (and I presume Siril), works? If you're shooting in mono, then clearly you load up each filter's images and assign them to their respective RBG channel. But what happens if you do channel extraction on OSC broadband data (apologies if this should be obvious to me, but it's not)? Does the software automatically assign wavelengths (via pixel values) to a channel? e.g. reddish pixels representing wavelengths in the 600-700 nm range to red, greenish pixels in the 500-600 nm range to green, etc.
What about dual (or tri) OSC narrow band data? There should then only be 2 (or 3) narrow spikes representing Ha, Oiii (and Sii) , which if you split into RGB channels gets assigned how?
I'm trying to understand because I really like some of the different colour palettes (especially Hubble) and would like to be able to emulate this (I know it's not colour-accurate as in shooting in mono might provide) with a colour camera. I see that you can almost get to true SHO (that a mono setup would provide) with some of the new filter sets using OSC (e.g. Askar D1/D2) - albeit faux-SHO.
If you've got any good resources to point me towards on colour palettes in astrophotography, I'd be appreciative.
Thanks,
Paul