Administrator
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The reported values are a relative measurement of the roundness (vs. eccentric due to tracking or guiding problems) of the stellar PSF in the aperture. The measurement is a by-product of the centroiding routine which provides estimates of the FWHM values in both the x-axis and y-axis directions. The roundness is then 1 - ecc, where ecc = ((xWidth-yWidth)*(xWidth-yWidth)+4.0*mxy*mxy)/((xWidth+yWidth)*(xWidth+yWidth)), and where mxy is a representation of the combined FWHM estimate. If you need more detailed information, you'll need to look at the AIJ code in Centroid.java starting at line 540.
Karen
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