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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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| Опубликовано в: : | Sensors (Basel) |
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| Главные авторы: | , , , , |
| Формат: | Artigo |
| Язык: | Inglês |
| Опубликовано: |
MDPI
2018
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| Предметы: | |
| Online-ссылка: | https://ncbi.nlm.nih.gov/pmc/articles/PMC6163372/ https://ncbi.nlm.nih.gov/pubmed/30154307 https://ncbi.nlm.nih.govhttp://dx.doi.org/10.3390/s18092836 |
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