I started a project on IC405 the Flaming Star Nebula collecting 60s RGB subframes the first couple of nights, then I inadvertently switched on subsequent nights to 30s subframes. I used a QHY163M CMOS camera/60mm doublet.
It's rather complex what I ended up with:
R 30s x199
60s x120
G 30s x56
60s x176
B 30s x108
60s x176
The total imaging time is similar: R (3.7h); G (3.4h); B (4h) but the balance of 30s and 60s subs for ea color is quite different.
How would you recommend processing these? Calibrate and stack all separately? Calibrate and stack ea color together (can I stack the 30s and 60s subs together for ea color)?
I also have nearly 10h of Ha taken with a different camera (Atik 383L)/telescope (90mm triplet) (smaller FOV but the image scales are similar: 2.2 arcsec/pixel for the Ha data; 3 arcsec/pixel for the color data). I'm thinking of using the Ha for luminance data (lots of resolution and texture) and blending it with the color data from the QHY163M.
Advice on how to approach this would be appreciated.
...Keith