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- W4250519385 abstract "Radioastronomical observations are often incomplete in the sense that either the angular resolution desired or the signal-to-noise ratio required are not adequate. Attempts to fill in the missing information by either smoothing or deconvolving the observed data date back to Bracewell (1956, 1958). More recently the need for more sophisticated restoration procedures has increased since observations with radioastronomical interferometers frequently suffer from incomplete coverage of the u – v plane. Procedures like CLEAN (Högbom 1974, Schwarz 1978) and MEM (Wernecke 1977, Gull and Daniell 1978) have been developed to interpolate the unknown data in the u – v plane." @default.
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- W4250519385 date "1979-01-01" @default.
- W4250519385 modified "2023-09-23" @default.
- W4250519385 title "The Information of Images and Its Dependence on Noise and Spatial Resolution" @default.
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- W4250519385 doi "https://doi.org/10.1017/s0252921100074959" @default.
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