


Until a couple of years ago, imagers who used separate guide scopes generally took it seriously: a real refractor telescope mounted close to the main OTA using a dovetail plate and two well-separated clamshell-type mounting rings for the guide scope. And they were also using guide cameras with larger pixels, in the range of 6-9 microns. They often went to extra lengths to be sure that one of the mounting points was close to the focuser and guide camera so those elements wouldn’t move around or sag. As a result, we generally didn’t see many problems with unwanted movement in the guiding assembly, so the ratio of image scales between guiding and imaging was the primary consideration. But now we’re in a new world of tiny-pixel cameras and slick sales campaigns that urge you to fasten your guide camera on the back of a finder-scope, a use it was probably never intended for. And more often than not, that little finder-scope is on a central stalk, probably poking a considerable distance above the main OTA, with a handful of thumbscrews to hold things tight. As a result, it can be a substantial source of instability. Even the hanging weight of a guide cable can cause the camera sensor to move by a few microns (you should try to visualize how small that is, a human hair is roughly 50 microns thick) and you can get a 6- 10 arc-sec guiding deviation as a result.
Good luck,
Bruce
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