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In order to produce high dynamic range images in radio interferometry, bright extended sources need to be removed with minimal error.
D. Slepian and H. O. Pollak, “Prolate spheroidal wave functions, Fourier analysis, and uncertainty-I,” Bell Syst. Tech. J. , vol. 40, no. 2, pp. 43–61, 1961
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H. J. Landau and H. O. Pollak, “Prolate spheroidal wave functions, Fourier analysis, and uncertainty-II,” Bell Syst. Tech. J. , vol. 40, no. 2, pp. 65–84, 1961
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M. A. Lindquist, C. Zhang, G. Glover, L. Shepp, and Q. X. Yang, “A generalization of the two dimensional prolate spheroidal wave function method for nonrectiliner MRI data acquisition methods,” IEEE Trans. on Image Proc. , vol. 15, no. 9, pp. 2792–2804, 2006
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S. Yatawatta, “Fundamental limitations of pixel based image deconvolution in radio astronomy,” in proc. IEEE Sensor Array and Multichannel Signal Processing Workshop (SAM), Israel , pp. 69–72, 2010
2010
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R. Levanda and A. Leshem, “Adaptive selective sidelobe canceller beamformer with applications in radio astronomy,” in proc. IEEE 26-th Convention of Electrical and Electronics Engineers (IEEEI), Israel , 2010
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F. J. Simons and D. V. Wang, “Spatiospectral conventration in the Cartesian plane,” Appl. Comput. Harmon. Anal. under review , 2010
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Later among the works it cites.
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