When observing a fuzzy comet there is a danger that presence of a coma and tails will drag a normal PSF measurement away from the true nucleus position. In Astrometrica, you can use the Centroid button and a normal (or larger) aperture setting to get a magnitude including as much coma as you like. Then use the Background and Range adjustment to reduce the comet image to a small cluster of bright pixels, change to a small aperture that will just fit the cluster, and make a measurement of position in the normal way. That should be the nucleus position.
The purpose of this page is to merge the separate position and magnitude observations into a single report for submission to the MPC.
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