Contents
- Index
Guiding Comments
Setting your maximum allowable error depends on many factors; seeing conditions, wind speed, the accuracy of your mount, the image scale of your imaging setup, etc. Finding the right balance of your systems capabilities and when you should issue a correction takes some experimentation. I have provided these illustrations to help with this process.
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In this common example, we see a situation where the seeing and mount accuracy of the imaging system are ~1.00 arc-seconds. The minimum movement is set very low at 0.30" arc-seconds. The guide star centroid is staying well within the systems capabilities, yet the autoguider relays are making unnecessary corrections leading to mount oscillations, over-corrections, unpredictable movements because of backlash, etc. In this example, the stellar profiles of the stars in the image are going to be distorted unnaturally because of poor autoguiding settings.
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By increasing our maximum allowable peak to peak error to 1 arc-second we only make corrections when the guide star centroid falls out of our systems capabilities i.e. when a correction is truly needed. As you can see we have reduced unnecessary guider corrections which will result in better stellar profiles and rounder stars.
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Here we have an example of the maximum allowable error being set to high. This could be the same imaging system on a night of excellent seeing or a different imaging system with a more accurate mount. As you can see, guide star centroids outside of our capabilities are not being corrected.
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By reducing the maximum allowable error to 0.60" arc-seconds, we are now correcting for the movements that fall out of our systems capabilities.