Study of centering CCD image of faint satellites near a bright primary object†

Details Study of centering CCD image of faint satellites near a bright primary object† Study of centering CCD image of faint satellites near a bright primary object†

Jul 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008iaus..248..138t&link_type=abstract

A Giant Step: from Milli- to Micro-arcsecond Astrometry, Proceedings of the International Astronomical Union, IAU Symposium, Vol

Astronomy and Astrophysics

Astronomy

Astrometry, Solar System: General, Techniques: Image Processing, Planets And Satellites: General

Scientific paper

The polynomial-fit method is applied to remove the uneven background of
a satellite when it is near a bright primary object. Detailed analysis
of this method is given. Some useful conclusions are drawn from the
results of simulated data.

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