Generation of realistic input parameters for simulating atmospheric point-spread functions at astronomical observatories
High-fidelity simulated astronomical images are an important tool in developing and measuring the performance of image-processing algorithms, particularly for high precision measurements of cosmic shear -- correlated distortions of images of distant galaxies due to weak gravitational lensing caused...
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| Principais autores: | , , , , |
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| Formato: | Artigo |
| Idioma: | Inglês |
| Publicado em: |
Maynooth Academic Publishing
2024-04-01
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| coleção: | The Open Journal of Astrophysics |
| Acesso em linha: | https://doi.org/10.33232/001c.115727 |
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