A New Layout Optimization Technique for Interferometric Arrays, Applied to the Murchison Widefield Array

Antenna layout is an important design consideration for radio interferometers because it determines the quality of the snapshot point spread function (PSF, or array beam). This is particularly true for experiments targeting the 21-cm Epoch of Reionization signal as the quality of the foreground subt...

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Main Authors: Beardsley, A.P., Hazelton, B.J., Morales, M.F., Capallo, R.J., Goeke, R., Emrich, D., Lonsdale, C.J., Arcus, W., Barnes, D., Bernardi, G., Bowman, J.D., Bunton, J.D., Corey, B.E., Deshpande, A., DeSouza, L., Gaensler, B.M., Greenhill, L.J., Herne, D., Hewitt, J.N., Kaplan, D.L., Kasper, J.C., Kincaid, B.B., Koenig, R., Kratzenberg, E., Lynch, M.J., McWhirter, S.R., Mitchell, D.A., Morgan, E., Oberoi, D., Ord, S.M., Pathikulangara, J., Prabu, T., Remillard, R.A., Rogers, A.E.E., Roshi, A., Salah, J.E., Sault, R.J., Udaya Shankar, N., Srivani, K.S., Stevens, J., Subrahmanyan, R., Tingay, Steven, Wayth, Randall, Waterson, M., Webster, R.L., Whitney, A.R., Williams, A., Wyithe, J.S.B.
Format: Journal Article
Published: Wiley-Blackwell Publishing Ltd. 2012
Subjects:
Online Access:http://hdl.handle.net/20.500.11937/44268
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author Beardsley, A.P.
Hazelton, B.J.
Morales, M.F.
Capallo, R.J.
Goeke, R.
Emrich, D.
Lonsdale, C.J.
Arcus, W.
Barnes, D.
Bernardi, G.
Bowman, J.D.
Bunton, J.D.
Corey, B.E.
Deshpande, A.
DeSouza, L.
Gaensler, B.M.
Greenhill, L.J.
Herne, D.
Hewitt, J.N.
Kaplan, D.L.
Kasper, J.C.
Kincaid, B.B.
Koenig, R.
Kratzenberg, E.
Lynch, M.J.
McWhirter, S.R.
Mitchell, D.A.
Morgan, E.
Oberoi, D.
Ord, S.M.
Pathikulangara, J.
Prabu, T.
Remillard, R.A.
Rogers, A.E.E.
Roshi, A.
Salah, J.E.
Sault, R.J.
Udaya Shankar, N.
Srivani, K.S.
Stevens, J.
Subrahmanyan, R.
Tingay, Steven
Wayth, Randall
Waterson, M.
Webster, R.L.
Whitney, A.R.
Williams, A.
Wyithe, J.S.B.
author_facet Beardsley, A.P.
Hazelton, B.J.
Morales, M.F.
Capallo, R.J.
Goeke, R.
Emrich, D.
Lonsdale, C.J.
Arcus, W.
Barnes, D.
Bernardi, G.
Bowman, J.D.
Bunton, J.D.
Corey, B.E.
Deshpande, A.
DeSouza, L.
Gaensler, B.M.
Greenhill, L.J.
Herne, D.
Hewitt, J.N.
Kaplan, D.L.
Kasper, J.C.
Kincaid, B.B.
Koenig, R.
Kratzenberg, E.
Lynch, M.J.
McWhirter, S.R.
Mitchell, D.A.
Morgan, E.
Oberoi, D.
Ord, S.M.
Pathikulangara, J.
Prabu, T.
Remillard, R.A.
Rogers, A.E.E.
Roshi, A.
Salah, J.E.
Sault, R.J.
Udaya Shankar, N.
Srivani, K.S.
Stevens, J.
Subrahmanyan, R.
Tingay, Steven
Wayth, Randall
Waterson, M.
Webster, R.L.
Whitney, A.R.
Williams, A.
Wyithe, J.S.B.
author_sort Beardsley, A.P.
building Curtin Institutional Repository
collection Online Access
description Antenna layout is an important design consideration for radio interferometers because it determines the quality of the snapshot point spread function (PSF, or array beam). This is particularly true for experiments targeting the 21-cm Epoch of Reionization signal as the quality of the foreground subtraction depends directly on the spatial dynamic range and thus the smoothness of the baseline distribution. Nearly all sites have constraints on where antennas can be placed even at the remote Australian location of the Murchison Widefield Array (MWA) there are rock outcrops, flood zones, heritages areas, emergency runways and trees. These exclusion areas can introduce spatial structure into the baseline distribution that enhances the PSF sidelobes and reduces the angular dynamic range. In this paper we present a new method of constrained antenna placement that reduces the spatial structure in the baseline distribution. This method not only outperforms random placement algorithms that avoid exclusion zones, but surprisingly outperforms random placement algorithms without constraints to provide what we believe are the smoothest constrained baseline distributions developed to date. We use our new algorithm to determine antenna placements for the originally planned MWA, and present the antenna locations, baseline distribution and snapshot PSF for this array choice.
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format Journal Article
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institution Curtin University Malaysia
institution_category Local University
last_indexed 2025-11-14T09:20:21Z
publishDate 2012
publisher Wiley-Blackwell Publishing Ltd.
recordtype eprints
repository_type Digital Repository
spelling curtin-20.500.11937-442682017-09-13T16:07:58Z A New Layout Optimization Technique for Interferometric Arrays, Applied to the Murchison Widefield Array Beardsley, A.P. Hazelton, B.J. Morales, M.F. Capallo, R.J. Goeke, R. Emrich, D. Lonsdale, C.J. Arcus, W. Barnes, D. Bernardi, G. Bowman, J.D. Bunton, J.D. Corey, B.E. Deshpande, A. DeSouza, L. Gaensler, B.M. Greenhill, L.J. Herne, D. Hewitt, J.N. Kaplan, D.L. Kasper, J.C. Kincaid, B.B. Koenig, R. Kratzenberg, E. Lynch, M.J. McWhirter, S.R. Mitchell, D.A. Morgan, E. Oberoi, D. Ord, S.M. Pathikulangara, J. Prabu, T. Remillard, R.A. Rogers, A.E.E. Roshi, A. Salah, J.E. Sault, R.J. Udaya Shankar, N. Srivani, K.S. Stevens, J. Subrahmanyan, R. Tingay, Steven Wayth, Randall Waterson, M. Webster, R.L. Whitney, A.R. Williams, A. Wyithe, J.S.B. miscellaneous cosmoloy interferometers instrumentation Antenna layout is an important design consideration for radio interferometers because it determines the quality of the snapshot point spread function (PSF, or array beam). This is particularly true for experiments targeting the 21-cm Epoch of Reionization signal as the quality of the foreground subtraction depends directly on the spatial dynamic range and thus the smoothness of the baseline distribution. Nearly all sites have constraints on where antennas can be placed even at the remote Australian location of the Murchison Widefield Array (MWA) there are rock outcrops, flood zones, heritages areas, emergency runways and trees. These exclusion areas can introduce spatial structure into the baseline distribution that enhances the PSF sidelobes and reduces the angular dynamic range. In this paper we present a new method of constrained antenna placement that reduces the spatial structure in the baseline distribution. This method not only outperforms random placement algorithms that avoid exclusion zones, but surprisingly outperforms random placement algorithms without constraints to provide what we believe are the smoothest constrained baseline distributions developed to date. We use our new algorithm to determine antenna placements for the originally planned MWA, and present the antenna locations, baseline distribution and snapshot PSF for this array choice. 2012 Journal Article http://hdl.handle.net/20.500.11937/44268 10.1111/j.1365-2966.2012.20878.x Wiley-Blackwell Publishing Ltd. fulltext
spellingShingle miscellaneous
cosmoloy
interferometers
instrumentation
Beardsley, A.P.
Hazelton, B.J.
Morales, M.F.
Capallo, R.J.
Goeke, R.
Emrich, D.
Lonsdale, C.J.
Arcus, W.
Barnes, D.
Bernardi, G.
Bowman, J.D.
Bunton, J.D.
Corey, B.E.
Deshpande, A.
DeSouza, L.
Gaensler, B.M.
Greenhill, L.J.
Herne, D.
Hewitt, J.N.
Kaplan, D.L.
Kasper, J.C.
Kincaid, B.B.
Koenig, R.
Kratzenberg, E.
Lynch, M.J.
McWhirter, S.R.
Mitchell, D.A.
Morgan, E.
Oberoi, D.
Ord, S.M.
Pathikulangara, J.
Prabu, T.
Remillard, R.A.
Rogers, A.E.E.
Roshi, A.
Salah, J.E.
Sault, R.J.
Udaya Shankar, N.
Srivani, K.S.
Stevens, J.
Subrahmanyan, R.
Tingay, Steven
Wayth, Randall
Waterson, M.
Webster, R.L.
Whitney, A.R.
Williams, A.
Wyithe, J.S.B.
A New Layout Optimization Technique for Interferometric Arrays, Applied to the Murchison Widefield Array
title A New Layout Optimization Technique for Interferometric Arrays, Applied to the Murchison Widefield Array
title_full A New Layout Optimization Technique for Interferometric Arrays, Applied to the Murchison Widefield Array
title_fullStr A New Layout Optimization Technique for Interferometric Arrays, Applied to the Murchison Widefield Array
title_full_unstemmed A New Layout Optimization Technique for Interferometric Arrays, Applied to the Murchison Widefield Array
title_short A New Layout Optimization Technique for Interferometric Arrays, Applied to the Murchison Widefield Array
title_sort new layout optimization technique for interferometric arrays, applied to the murchison widefield array
topic miscellaneous
cosmoloy
interferometers
instrumentation
url http://hdl.handle.net/20.500.11937/44268