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Cited by 431

The DOI matches its Crossref record; 43 of the 43 references it cites were found in a registry or an index.

Deconvolution in Astronomy: A Review

Open access
Starck, J. L., Pantin, E., Murtagh, F.·2002·Publications of the Astronomical Society of the Pacific

Abstract

This article reviews different deconvolution methods. The all‐pervasive presence of noise is what makes deconvolution particularly difficult. The diversity of resulting algorithms reflects different ways of estimating the true signal under various idealizations of its properties. Different ways of approaching signal recovery are based on different instrumental noise models, whether the astronomical objects are pointlike or extended, and indeed on the computational resources available to the analyst. We present a number of recent results in this survey of signal restoration, including in the areas of superresolution and dithering. In particular, we show that most recent published work has consisted of incorporating some form of multiresolution in the deconvolution process.

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Metadata

Authors
Starck, J. L., Pantin, E., & Murtagh, F.
Venue
Publications of the Astronomical Society of the Pacific
Published
2002-10
Volume
114
Issue
800
Pages
1051-1069
ISSN
  • 0004-6280 (ISSN-L)
  • 1538-3873
OpenAlex
W2011687187
Cited by
431
References
43
FWCI
12.36
Type
journal article
Language
en
Open access
bronze

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CoChat. (2026). Citation check: Deconvolution in Astronomy: A Review. https://app.cochat.ai/papers/10.1086/342606
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Starck, J. L., Pantin, E., & Murtagh, F. (2002). Deconvolution in Astronomy: A Review. Publications of the Astronomical Society of the Pacific. https://doi.org/10.1086/342606

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