Re: Accuracy of Centroid Measurement
Posted by
karenacollins on
Oct 06, 2014; 10:18pm
URL: http://astroimagej.170.s1.nabble.com/Accuracy-of-Centroid-Measurement-tp184p185.html
Hi Dave,
As far as the accuracy of the centroid measurement, I don't have
much information to offer. I think it would depend on several
factors, including star brightness and PSF shape (e.g. focused vs.
defocused). Also, the measured centroid location depends somewhat on
where the starting point is relative to the final determined
centroid location. However, the "Howell" centroid option (see below)
gives very repeatable results, no matter where the starting point is
(within reason). Do you have the "Howell centroid method" enabled or
disabled in aperture settings?
AIJ currently reports all measurements using 6 decimal places, so
there is no intended precision due to the number of reported decimal
places.
There are actually two different methods of centroiding in AIJ,
which can be selected by clicking the "Change Aperture Settings"
icon (

)
above an image. That will open the panel shown below (from AIJ
version 2.1.5). If "Use Howell centroid method" is DESELECTED, a
basic "Center of mass (light)" calculation is done to find the
centroid. If SELECTED, the method described in Howell, CCD
Astronomy, 2nd Ed., p. 105 is implemented. Both of these methods
require iteration to settle on the best centroid point. They both
work about the same for focused stars, except that the Howell method
finds almost the exact same centroid with fewer iterations, no
matter which side of the PSF it is the starting from. The Howell
method works best if you have focused and/or faint stars and you
want to get consistent centroid results every time. If you have
brighter stars with defocused doughnuts that are not exactly
symmetrical in brightness around the doughnut, the "non-Howell"
version finds a centroid that is a little closer to the center of
the doughnut, which I think is what is desired in that case.
If you are able to characterize the precision, in one or both
centroid modes, I would be interested to know about your findings,
once they are public.
Karen