Star Centroiding Based on Fast Gaussian Fitting for Star Sensors

The most accurate star centroiding method for star sensors is the Gaussian fitting (GF) algorithm, because the intensity distribution of a star spot conforms to the Gaussian function, but the computational complexity of GF is too high for real-time applications. In this paper, we develop the fast Ga...

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Detalles Bibliográficos
Autores principales: Wan, Xiaowei, Wang, Gangyi, Wei, Xinguo, Li, Jian, Zhang, Guangjun
Formato: Online Artículo Texto
Lenguaje:English
Publicado: MDPI 2018
Materias:
Article
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC6163372/
https://www.ncbi.nlm.nih.gov/pubmed/30154307
http://dx.doi.org/10.3390/s18092836

Internet

https://www.ncbi.nlm.nih.gov/pmc/articles/PMC6163372/
https://www.ncbi.nlm.nih.gov/pubmed/30154307
http://dx.doi.org/10.3390/s18092836

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