The applications of digital centering algorithms have a major impact on precise astrometry. In optical observations of space debris, due to the observing strategies and methods, the image degradation is distinct, which affects the centroid computing of CCD images. Adopting the four widely-used centering algorithms, including modified moment, one-dimensional Gaussian fit, two-dimensional Gaussian fit and median, tests are made on raw CCD images of space debris. With the observation positions obtained by astronomical calibration and the reference ones from ephemeris, the precision of variable algorithms and the influence of different threshold settings are acquired. The results indicate that the median reveals performs best for right ascension coordinates and others reveals a better results for declination coordinates. For Gaussian fit, no threshold may improve the centering precision.
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