This project fell on hard times after I was able to complete the infrastructure for switching cameras on the fly and implementing a custom exposure hook. It resulted in the addition of a new Custom Action method in ACP 8.1 for support. The project stalled at the point where we needed to identify the target star in the spectrograph's guider field of view, as well identifying the XY coordinates of the fiber within said guider's field. I believe she was able to make an engineering improvement such that the fiber location stays constant. Identifying the target star, however, remains to be solved.

I added the above because another customer is looking to do this with a different spectrograph (different challenges). I am closing this mis-named thread so he can start a fresh one.