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...

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Bibliographic Details
Main Authors: Suszyński Robert, Wawryn Krzysztof
Format: Article
Language:English
Published: Polish Academy of Sciences 2015-12-01
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