I'm setting up an RC8 to mount in my small remote private observatory. I have documented a lot about the guide for important focal lengths such as the full native one of the RC 8. Most recommend an OAG ….. I think I understand that to do this, especially from a remote observatory, you need a sensor up to it, so not inferior to a Lodestar or an ASI 174 MM mini. This is because remotely you must be sure to see the star always, not being able to act on the prism in both rotation and angle. We are therefore talking about top but expensive CCD. Now to start I will definitely rely on the guide with tele-guide and the trusty SSAG, then we'll see ….. My question is: will I have problems at 1.624 focal length to get the round stars? Making sure that there are no flexions between the guide ota and the main ota, nor flexions of the fok of the tele-guide because in general the guide with tele-guide is considered more poor than the OAG? Often with the OAG you drive on deformed and low quality stars ….. so I would like to understand well if there is a technical / scientific reason …. I know with the OAG you drive a star almost inside the sensor field , while in the other way no ….. but what changes?