Stars’ Centroid Determination Using PSF-Fitting Method
This paper presents an algorithm for restoring telescope images corrupted by turbulence effects and readout noise of a telescope system in order to determine centroid positions of stars, especially the position of a reference star. A computation method employing an accurate centroid estimation algor...
Main Authors: | , |
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Format: | Article |
Language: | English |
Published: |
Polish Academy of Sciences
2015-12-01
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Series: | Metrology and Measurement Systems |
Subjects: | |
Online Access: | http://www.degruyter.com/view/j/mms.2015.22.issue-4/mms-2015-0047/mms-2015-0047.xml?format=INT |