2022
DOI: 10.1016/j.actaastro.2021.12.046
|View full text |Cite
|
Sign up to set email alerts
|

Centroid determination based on energy flow information for moving dim point targets

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
1

Citation Types

0
2
0

Year Published

2022
2022
2024
2024

Publication Types

Select...
4
2

Relationship

0
6

Authors

Journals

citations
Cited by 10 publications
(2 citation statements)
references
References 28 publications
0
2
0
Order By: Relevance
“…The luminance distribution of a star in the star image depends on the point spread function (PSF) and the position of the star. In common with many previous studies, [8][9][10][11] 2D Gaussian PSF is used. In order to obtain the simulating verisimilitude about the earth observing sensors, the gray diffusion also needs to be done with each of the star image spots.…”
Section: Image Simulationmentioning
confidence: 99%
“…The luminance distribution of a star in the star image depends on the point spread function (PSF) and the position of the star. In common with many previous studies, [8][9][10][11] 2D Gaussian PSF is used. In order to obtain the simulating verisimilitude about the earth observing sensors, the gray diffusion also needs to be done with each of the star image spots.…”
Section: Image Simulationmentioning
confidence: 99%
“…However, Thomas et al [23] found that when the signal to noise ratio (SNR) did not meet the tracking conditions, the cross-correlation function could not seek the optimal solution, and the tracking spot target morphology was greatly affected by random noise. In 2021, Sun et al [24] proposed a filtered centering method based on the motion pattern which can effectively solve the problem of random noise. However, this algorithm requires continuous motion information of the point target and is not real-time [25].…”
mentioning
confidence: 99%