Compressed sensing imaging techniques for radio interferometry
Compressed sensing imaging techniques for radio interferometry
Radio interferometry probes astrophysical signals through incomplete and noisy Fourier measurements. The theory of compressed sensing demonstrates that such measurements may actually suffice for accurate reconstruction of sparse or compressible signals. We propose new generic imaging techniques based on convex optimization for global minimization problems defined in this context. The versatility of the framework notably allows introduction of specific prior information on the signals, which offers the possibility of significant improvements of reconstruction relative to the standard local matching pursuit algorithm CLEAN used in radio astronomy. We illustrate the potential of the approach by studying reconstruction performances on simulations of two different kinds of signals observed with very generic interferometric configurations. The first kind is an intensity field of compact astrophysical objects. The second kind is the imprint of cosmic strings in the temperature field of the cosmic microwave background radiation, of particular interest for cosmology
1733-1742
Wiaux, Y.
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Jacques, L.
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Puy, G.
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Scaife, A.M.M.
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Vandergheynst, P.
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May 2009
Wiaux, Y.
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Jacques, L.
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Puy, G.
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Scaife, A.M.M.
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Vandergheynst, P.
d72f3902-a4fb-44b9-a394-cc130e36a803
Wiaux, Y., Jacques, L., Puy, G., Scaife, A.M.M. and Vandergheynst, P.
(2009)
Compressed sensing imaging techniques for radio interferometry.
Monthly Notices of the Royal Astronomical Society, 395 (3), .
(doi:10.1111/j.1365-2966.2009.14665.x).
Abstract
Radio interferometry probes astrophysical signals through incomplete and noisy Fourier measurements. The theory of compressed sensing demonstrates that such measurements may actually suffice for accurate reconstruction of sparse or compressible signals. We propose new generic imaging techniques based on convex optimization for global minimization problems defined in this context. The versatility of the framework notably allows introduction of specific prior information on the signals, which offers the possibility of significant improvements of reconstruction relative to the standard local matching pursuit algorithm CLEAN used in radio astronomy. We illustrate the potential of the approach by studying reconstruction performances on simulations of two different kinds of signals observed with very generic interferometric configurations. The first kind is an intensity field of compact astrophysical objects. The second kind is the imprint of cosmic strings in the temperature field of the cosmic microwave background radiation, of particular interest for cosmology
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e-pub ahead of print date: 8 April 2009
Published date: May 2009
Organisations:
Astronomy Group
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Local EPrints ID: 336936
URI: http://eprints.soton.ac.uk/id/eprint/336936
ISSN: 1365-2966
PURE UUID: 17b77a62-7abf-4742-a885-d41153597751
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Date deposited: 31 May 2012 11:06
Last modified: 14 Mar 2024 10:47
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Author:
Y. Wiaux
Author:
L. Jacques
Author:
G. Puy
Author:
A.M.M. Scaife
Author:
P. Vandergheynst
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