CHriss I've ordered a QHY5III 178 Mono as guide cam
Do you still have time to exchange it for the QHY5III 678 Mono camera?
The IMX678 is more sensitive than the IMX178 sensor, and at the same time have 2 µm pixels instead of 2.9 µm. Additionally, the QHY camera comes with an IR-pass (685 if memory serves) filter in the box so you can try near-IR guiding too (for me, I get a 25% better guiding with near IR and I get better improvements with other tweaks, so I have myself put near IR guiding on the side -- getting more stars is more important). The pixels are half the size of one from an ASI220.
Getting lots of stars with lots of gain margin available (i.e., being able to push 20 dB past 12 stars) is important because, if I am not wrong, PHD2 uses SNR weighted centroids. The proper thing to do is to use a different weight. But we do not have a choice if we don't write our own software.
Just the the past week, a Forum reader had asked to read the white paper that I was working on. I confessed that I have not touched that (waiting for winter when it is clouded up and rains for 3 mounts non stop to resume) but made a checkpoint of what I currently have (rough notes all over and very rough English -- was my third language):
http://www.w7ay.net/site/Downloads/AutoGuiding/Rough/index.html
Scroll to section "Appendix B. Star Centroids Under Atmospheric Turbulence" and you will find how pushing the gain helps when the guide software mistakenly uses SNR as the centroiding weight.
Again, I apologize for the very rough nature of the whole paper.
I use an ASI178MM with ASIAIR, but have started to experiment with my own autoguiding algorithms using the QHY678M and INDIGO (macOS desktop, with M1 Mac Mini [modified for 12V] or Raspberry Pi 4 at the telescope). No definitive result yet, but I expect the 678 to comfortably outshoot the 178. Definitely searching for a better centroid weight (I suspect for now it is simply uniform weighting since centroid error is not much affected by SNR).
I already use a high quality 60mm f/4 scope for guiding
Take a well focused image from it and look at the FHWM or HFD over the frame. Are the star sizes within 10% from one another? Even the best refractor objective has field curvature, and we do need the star shapes to be moderately uniform to take full advantage of multi-star centroid estimation. The world has changed from the single star case, where you can pick just a single good guide star. And for the sake of the stars away from the optical axis, you need to focus well (I have a belt driven EAF on my guide scope since I am too lazy to spend time outdoors in the dark and cold fiddling with a helical focuser).
Chen