I’ll put my $0.02 in here with support for the dual scope idea.
I currently run 2 scopes/cameras side by side and really have no issues with it. My seeing is also quite bad, and I found larger aperture fast scopes seemed to be more prone to bad seeing and wind and were more fiddly with tilt and since I didn’t have narrowband filters that were designed for fast scopes, I wasn’t getting the most out of it. I didn’t switch to fast filters since I used the camera on multiple scopes. And one scope /camera locks you into one focal length (or mess with various reducers and such.
My strategy was to use a longer refractor (I started with the Askar 140, now use the Tak TOA-130 which is incredible) and a wider refractor (WO Cat 91 which is great as well). I have a FF mono camera and a OSC APSC camera. If the target fits in the FF FOV of the longer scope, then it would fit in the FOV of APSC of the wider one.
I run them side-by-side on my Mach 2. I don’t guide and use Dec Arc modeling, which simplifies things a great deal. THe side by side setup with solid rings seems to work quite well, and my small scope APSC FOV is a bit wider than my Large scope FF, so allows for some small misalignment.
The best use case is broadband targets, where I capture luminance with the larger Mono FF scope and RGB with the smaller APSC OSC one. The mismatch in resolution is no big deal since color resolution isn’t nearly as important.
I run a mini PC with 2 instances of Nina, one master for the larger scope which controls mount and guiding/dithering and the other that just runs the camera/AF/rotation for the smaller APSC OSC. I use synchronized dithering which, for the most part, works great as long as everything runs smoothly. You just have to make sure your dithering # of frames * exposure/frame match on each instance (so one could be 180seconds dithering every frame and the other could be 60 seconds dithering every 3 frames) so no instance waits on the other more than a second or 2. Dithering using direct guide (since I’m not actually guiding) in Nina is super quick. I try to align when I need to AF as well to avoid waiting on each other.
I use PI WBPP to calibrate, align and stack and it actually works quite seamlessly. It automatically scales up and aligns the APSC frames to match the FF frames (you have to tell it to use a FF frame as the reference image). Once it chugs through all the frames, you have a full set of LRGB just as if you took them all with the same setup. Really not much more difficult than having one rig.
I experimented with narrowband and right now it’s use case isn’t as clear since you really can’t effectively get a balanced mono “lum” for narrowband. My next experiment is to use the FF scope for Ha and Sii and the wide one with a dual narrowband filter and extract the B&G channels for Oiii. This would only be beneficial for targets where Oiii doesn’t hold the majority of detail as Ha and Sii. Veil wouldn’t work as well, but many targets would. Going to try that tonight.
One advantage is I can move the FF camera over to the wider scope for wide vistas without unmounting and mounting scopes. I can also put my small SQA55 on top of my TOA130 and run the Cat91 FF L and SQA55 APSC RGB if I want to capture a wider field.
To the disadvantages:
Expensive! Need a very beefy mount, 2 cameras and 2 scopes (at least) plus probably a power/USB box (I use Wandererastro power pro v3). For PC, I use a Quieter 4c and it handles everything fine. A motor rotator on both is super helpful in keeping the FOVs the same.
Not very portable. I image from my driveway and roll the whole rig out so not a big deal for me.
If something goes wrong and Nina gets out of sync with the synced dithering, one side may be waiting on the other more than expected. Happened more often as I was learning.
If your scope geometries don’t match (barrel or pincushion), you’ll need to use slower alignment methods in WBPP to get stars to match throughout the frame. My current scopes (TOA130 & CAT 91) match very well
I won’t say having more exposures, since faster scopes generally require shorter exposure times.
Doesn’t synchronize meridian flip, so lose an exposure on the non-master instance
Here’s some examples I’ve done using the L/RGB method:
https://app.astrobin.com/u/Ricksastro?i=or2t0h#gallery
https://app.astrobin.com/u/Ricksastro?i=roaf6s#gallery
https://app.astrobin.com/u/Ricksastro?i=h4w8j5#gallery
https://app.astrobin.com/u/Ricksastro?i=4a8kl2#gallery
📷 IMG_5915.jpeg