Author Affiliations
1Yunnan Observatories, Chinese Academy of Sciences, Kunming 650216, Yunnan, China2University of Chinese Academy of Sciences, Beijing 100049, China3Key Laboratory of Space Object & Debris Observation, Chinese Academy of Sciences, Nanjing 210034, Jiangsu, Chinashow less
Fig. 1. Definition of FWHM
Fig. 2. HFD of different type of images. (a) Noise image; (b) faint star; (c) star in focus
Fig. 3. Algorithm flow chart
Fig. 4. Comparison of images before and after anisotropic diffusion method processing. (a) Original image; (b) image after processing
Fig. 5. Comparison of images before and after Qtsu algorithm processing. (a) Original image; (b) image after processing
Fig. 6. Comparison of images before and after cluster algorithm processing. (a) Original image; (b) image after processing
Fig. 7. Performance comparison of algorithms. (a) Performance comparison of algorithms under different noise when FWHM is constant; (b) performance comparison of algorithms under different spot sizes when SNR is constant
Fig. 8. Partial image sequences of object 33320
Fig. 9. Outlier detection
Fig. 10. FWHM values obtained by fitting for different frames of image numbered 33320 (arrow points to direction of increase of i)
Fig. 11. Focusing curve fitted with measured FWHM
Fig. 12. HFD of different image frames in target numbered 33320
Fig. 13. V-shaped focusing curves after fitting
Method | FWHM | HFD | HFD-ICA | IRAF |
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Focusing ratio /% | 90 | 94 | 98 | 98 |
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Table 1. Comparison of precise focusing ratios
Noise percentage /% | 0 | 1 | 2 | 3 | 4 | 5 | 10 |
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| FWHM | 90 | 90 | 88 | 88 | 86 | 86 | 84 | HFD | 94 | 94 | 92 | 92 | 90 | 90 | 88 | HFD-ICA | 98 | 98 | 98 | 98 | 98 | 98 | 96 | IRAF | 98 | 98 | 98 | 98 | 96 | 94 | 94 |
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Table 2. Comparison of precise focusing ratio with noise disturbance
Parameter | Min time | Max time | Mean time |
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FWHM | 22.4 | 38.9 | 32.4 | HFD | 11.6 | 16.7 | 14.3 | HFD-ICA | 3.6 | 5.8 | 4.7 | IRAF | 32.4 | 48.6 | 45.7 |
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Table 3. Comparison of computing time of four algorithms unit: s