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Cited by 359

The DOI matches its Crossref record; 1 of the 1 references it cites were found in a registry or an index.

Image Formation by Self-Calibration in Radio Astronomy

Pearson, T. J., Readhead, A. C. S.·1984·Annual Review of Astronomy and Astrophysics

Abstract

This review describes these self-calibration methods and their application to both conventional and very long baseline arrays and includes examples of the high-quality images that they produce. After first defining closure phase and closure amplitude in Section 2, we review conventional aperture synthesis methods in Sections 3 and 4. The new iterative self-calibration algorithms are the subject of Section 5. In Section 6 we consider the capabilities and limitations of these algorithms. Finally, in Section 7 we mention some applications in optical and infrared astronomy and in new radio instruments presently planned or under construction.

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Crossref · 10.1146/annurev.aa.22.090184.000525

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Metadata

Authors
Pearson, T. J., & Readhead, A. C. S.
Venue
Annual Review of Astronomy and Astrophysics
Published
1984-09
Volume
22
Issue
1
Pages
97-130
ISSN
  • 0066-4146 (ISSN-L)
  • 1545-4282
OpenAlex
W2173563237
Cited by
359
References
1
FWCI
11.73
Type
journal article
Language
en
Open access
closed

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CoChat. (2026). Citation check: Image Formation by Self-Calibration in Radio Astronomy. https://app.cochat.ai/papers/10.1146/annurev.aa.22.090184.000525
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Pearson, T. J., & Readhead, A. C. S. (1984). Image Formation by Self-Calibration in Radio Astronomy. Annual Review of Astronomy and Astrophysics. https://doi.org/10.1146/annurev.aa.22.090184.000525

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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).

Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.