- Edited
Skylab1 those are good numbers
Keep in mind that the native periodic error of my RST-135 mount is about 70 arc seconds peak-to-peak. Since it is mostly sinusoidal (with a small third harmonic), this translates to an unguided error of a whopping 25" RMS; you can't even take short unguided exposures with a fisheye lens! This is probably the highest periodic error of any mount sold over $1000.
The Harmonic Drive (strain wave gears) has all the nice properties (lightweight, lots of torque and thus requires no counterweights, virtually no backlash), but it also comes with large periodic errors. It has been used mainly for robotic arms and even to drive the wheels of the original Mars Rover; applications that don't require small periodic errors, while torque is king.
The darn thing is machined from a block of aluminum, and not a cast part. Even the serial number is laser etched. I have had mine outdoors (covered just with dry bags when not in use) 24/7 for the past year where it had sat outside through rain and snow. It is built like a tank, except it does not weigh like a tank.
On paper, it should be easy to guide it down as long as one uses a fast update to match the time derivative of the periodic error. It needs a 0.5 second exposure time, or less.
Therein lies the rub -- under typical seeing conditions, the centroid of a single star jitters so much that one typically needs to use 2 or more second to average the turbulence out. But a 2 second update time (the fastest you can get with a 2 second exposure), is too long to get the guided error of the RST-135 to go lower than 1" or so.
Multi-star guiding changes all that by allowing 0.5 second exposures since the use of multiple stars reduces the centroid variances in lieu of longer exposures.
The result appears to show that the mount indeed works quite well with even the experimental Multi-Star autoguiding in ASIAIR, reducing the 25" native error down to 0.5".
Your mount's problem may not be coming from a case where it needs a short guide exposure time, or even from lousy centroid estimates. I.e., the centroid error could have been reduced by using longer exposures instead of using more stars, which presumably, you have tried already, or by inspecting the PHD2 Guide assistant numbers.
Perhaps I should repeat what Multi-star guiding does and does not do: what it does is to achieve the equivalent (or even better) centroid estimates without requiring a long exposure time. It does not do anything else, although some of the other problems may not rear their heads when there are no extraneous bogus guide pulses that are caused by poor centroid estimates.
If the PHD2 Guide Assistant recommends a smaller MinMo than 0.2 pixels, then v1.6 will have something for you, independent of whether Multi-star guiding is of any use for your mount.
Chen