Subpixel centroiding algorithm for EMCCD star tracker

2008 ◽  
Author(s):  
Yufeng Li ◽  
Dongmei Li ◽  
Yanbo Liang
2003 ◽  
Vol 53 (2) ◽  
pp. 135-147 ◽  
Author(s):  
Giancarlo Rufino ◽  
Domenico Accardo

1994 ◽  
Author(s):  
Philip C. Thomas ◽  
Gangan Prathap ◽  
V. Koteswara Rao ◽  
Yashwant K. Jain
Keyword(s):  

1991 ◽  
Author(s):  
Isabella T. Lewis ◽  
Arno G. Ledebuhr ◽  
Timothy S. Axelrod ◽  
Scott A. Ruddell

1991 ◽  
Author(s):  
Isabella T. Lewis ◽  
Arno G. Ledebuhr ◽  
Timothy S. Axelrod ◽  
Joseph F. Kordas ◽  
Robert Hills

2013 ◽  
Vol 722 ◽  
pp. 187-193
Author(s):  
Xiao Fang Zhao ◽  
Guang Bin Liu ◽  
Chao Shan Liu

In order to realize the simulation testing and calibration of star tracker in the lab, a simulation algorithm for dynamic and celestial sphere star image was proposed. This algorithm could complete simulation of star image at any time and any visual axis point, also could realize in-orbit simulation according to a given track. A new method of space district dividing was also presented in order to improve the traditional method of space district dividing by ascension and declination, fully considered declination arc length gradually shortened with latitude increasing. It can remarkably enhance the updating frequency simulation star image.


2011 ◽  
Vol 50 (12) ◽  
pp. 1735 ◽  
Author(s):  
Hai-bo Liu ◽  
Jian-kun Yang ◽  
Jiong-qi Wang ◽  
Ji-chun Tan ◽  
Xiu-jian Li

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