Neural Network Based Point Spread Function Deconvolution For Astronomical Applications
Optical astronomical images are strongly affected by the point spread function (PSF) of the optical system and the atmosphere (seeing) which blurs the observed image. The amount of blurring depends both on the observed band, and on the atmospheric conditions during observation. A typical astronomica...
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| Autori principali: | , , , , , |
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| Natura: | Artigo |
| Lingua: | Inglês |
| Pubblicazione: |
Maynooth Academic Publishing
2023-08-01
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| Serie: | The Open Journal of Astrophysics |
| Accesso online: | https://doi.org/10.21105/astro.2210.01666 |
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