# name
Benefits of Image Deconvolution in CCD Imagery

# metadata.dc.description.abstract[].value
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.

# metadata.dc.publisher[].value
Instituto de Astronomi?a, Universidad Nacional Auto?noma de Me?xico.

# metadata.dc.relation.ispartof[].value
Revista Mexicana de Astronomía y Astrofísica, 2006, vol. 25, p. 50-52

# metadata.dc.rights[].value
(c) Instituto de Astronomía, Universidad Nacional Autónoma de México, 2006

# metadata.dc.source[].value
Articles publicats en revistes (Física Quàntica i Astrofísica)

# metadata.dc.title[].value
Benefits of Image Deconvolution in CCD Imagery