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Paper: Imaging with non-coplanar data
Volume: 19, Radio Interferometry: Theory, Techniques, and Applications, IAU Colloquium 131
Page: 184
Authors: Perley, R. A.; Cornwell, T. J.
Abstract: The general relation between interferometric data and sky brightness requires the use of 3D Fourier transforms. Only in special cases does the standard 2D Fourier relations result in images free of distortions. For the VLA, use of 2D transforms introduces errors which are important at low frequencies and high resolutions. Options and progress in solving the computational problems associated with the full solution are revised.
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