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dc.contributor.authorYoung, A.
dc.contributor.authorWijnholds, S.
dc.contributor.authorCarozzi, T.
dc.contributor.authorMaaskant, R.
dc.contributor.authorIvashina, M.
dc.contributor.authorDavidson, David
dc.date.accessioned2018-12-13T09:11:47Z
dc.date.available2018-12-13T09:11:47Z
dc.date.created2018-12-12T02:47:12Z
dc.date.issued2015
dc.identifier.citationYoung, A. and Wijnholds, S. and Carozzi, T. and Maaskant, R. and Ivashina, M. and Davidson, D. 2015. Efficient correction for both direction-dependent and baseline-dependent effects in interferometric imaging: An A-stacking framework. Astronomy and Astrophysics. 577.
dc.identifier.urihttp://hdl.handle.net/20.500.11937/71936
dc.identifier.doi10.1051/0004-6361/201425492
dc.description.abstract

© 2015 ESO. A general framework is presented for modeling direction-dependent effects that are also baseline-dependent, as part of the calibration and imaging process. Within this framework such effects are represented as a parametric linear model in which basis functions account for direction dependence, whereas expansion coefficients account for the baseline dependence. This separation enables the use ofa multiple fast Fourier transform-based implementation of the forward calculation (sky to visibility) in a manner similar to the W-stacking solution for non-coplanar baselines, and offers a potential improvement in computational efficiency in scenarios where the gridding operation in a convolution-based approach to direction-dependent effects may be too costly. Two novel imaging approaches that are possible within this framework are also presented.

dc.publisherEDP Sciences
dc.titleEfficient correction for both direction-dependent and baseline-dependent effects in interferometric imaging: An A-stacking framework
dc.typeJournal Article
dcterms.source.volume577
dcterms.source.issn0004-6361
dcterms.source.titleAstronomy and Astrophysics
curtin.departmentCurtin Institute of Radio Astronomy (Engineering)
curtin.accessStatusFulltext not available


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