Benefits of Image Deconvolution in CCD Imagery
We show how wavelet-based image deconvolution can provide to wide-field CCD telescopes an increase in limiting magnitude of Δ R ∼ 0.6 and significant deblending improvement. Astrometric accuracy is not distorted, therefore, the feasibility of the technique for astrometric projects is validated. We a...
| Autores: | , , , , , |
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| Tipo de recurso: | artículo |
| Estado: | Versión publicada |
| Fecha de publicación: | 2006 |
| País: | España |
| Institución: | Varias* (Consorci de Biblioteques Universitáries de Catalunya, Centre de Serveis Científics i Acadèmics de Catalunya) |
| Repositorio: | Recercat. Dipósit de la Recerca de Catalunya |
| OAI Identifier: | oai:recercat.cat:2445/228315 |
| Acceso en línea: | https://hdl.handle.net/2445/228315 |
| Access Level: | acceso abierto |
| Palabra clave: | Refracció astronòmica Fotometria astronòmica Telescopis Astronomical refraction Astronomical photometry Telescopes |
| Sumario: | We show how wavelet-based image deconvolution can provide to wide-field CCD telescopes an increase in limiting magnitude of Δ R ∼ 0.6 and significant deblending improvement. Astrometric accuracy is not distorted, therefore, the feasibility of the technique for astrometric projects is validated. We apply the deconvolution process to a set of images from the recently refurbished Baker-Nunn camera at Rothney Astrophysical Observatory. |
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