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dc.contributor.authorWilliams, Christopher Leigh
dc.contributor.authorGoeke, Robert F
dc.contributor.authorHewitt, Jacqueline N
dc.contributor.authorMorgan, Edward H
dc.contributor.authorRemillard, Ronald A
dc.date.accessioned2013-01-10T19:14:06Z
dc.date.available2013-01-10T19:14:06Z
dc.date.issued2012-10
dc.date.submitted2012-04
dc.identifier.issn0004-637X
dc.identifier.issn1538-4357
dc.identifier.urihttp://hdl.handle.net/1721.1/76242
dc.description.abstractWe introduce the Fast Holographic Deconvolution method for analyzing interferometric radio data. Our new method is an extension of A-projection/software-holography/forward modeling analysis techniques and shares their precision deconvolution and wide-field polarimetry, while being significantly faster than current implementations that use full direction-dependent antenna gains. Using data from the MWA 32 antenna prototype, we demonstrate the effectiveness and precision of our new algorithm. Fast Holographic Deconvolution may be particularly important for upcoming 21 cm cosmology observations of the Epoch of Reionization and Dark Energy where foreground subtraction is intimately related to the precision of the data reduction.en_US
dc.description.sponsorshipNational Science Foundation (U.S.) (Grant AST CAREER-0847753)en_US
dc.description.sponsorshipNational Science Foundation (U.S.) (Grant AST-1003314)en_US
dc.description.sponsorshipNational Science Foundation (U.S.) (Grant AST-0457585)en_US
dc.description.sponsorshipNational Science Foundation (U.S.) (Grant AST-1008353)en_US
dc.description.sponsorshipNational Science Foundation (U.S.) (Grant AST-0908884)en_US
dc.description.sponsorshipNational Science Foundation (U.S.) (Grant PHY-0835713)en_US
dc.description.sponsorshipAustralian Research Council (Grant LE0775621)en_US
dc.description.sponsorshipAustralian Research Council (Grant LE0882938)en_US
dc.description.sponsorshipUnited States. Air Force Office of Scientific Research (Grant FA9550-0510247)en_US
dc.description.sponsorshipMIT School of Scienceen_US
dc.language.isoen_US
dc.publisherIOP Publishingen_US
dc.relation.isversionofhttp://dx.doi.org/10.1088/0004-637X/759/1/17en_US
dc.rightsCreative Commons Attribution-Noncommercial-Share Alike 3.0en_US
dc.rights.urihttp://creativecommons.org/licenses/by-nc-sa/3.0/en_US
dc.sourcearXiven_US
dc.titleFast holographic deconvolution: a new technique for precision radio interferometryen_US
dc.typeArticleen_US
dc.identifier.citationSullivan, I. S. et al. “Fast holographic deconvolution: a new technique for precision radio interferometry.” The Astrophysical Journal 759.1 (2012): 17.en_US
dc.contributor.departmentMIT Kavli Institute for Astrophysics and Space Researchen_US
dc.contributor.mitauthorGoeke, Robert F.
dc.contributor.mitauthorHewitt, Jacqueline N.
dc.contributor.mitauthorMorgan, Edward H.
dc.contributor.mitauthorRemillard, Ronald Alan
dc.contributor.mitauthorWilliams, Christopher Leigh
dc.relation.journalAstrophysical Journalen_US
dc.eprint.versionAuthor's final manuscripten_US
dc.type.urihttp://purl.org/eprint/type/JournalArticleen_US
eprint.statushttp://purl.org/eprint/status/PeerRevieweden_US
dspace.orderedauthorsSullivan, I. S.; Morales, M. F.; Hazelton, B. J.; Arcus, W.; Barnes, D.; Bernardi, G.; Briggs, F. H.; Bowman, J. D.; Bunton, J. D.; Cappallo, R. J.; Corey, B. E.; Deshpande, A.; deSouza, L.; Emrich, D.; Gaensler, B. M.; Goeke, R.; Greenhill, L. J.; Herne, D.; Hewitt, J. N.; Johnston-Hollitt, M.; Kaplan, D. L.; Kasper, J. C.; Kincaid, B. B.; Koenig, R.; Kratzenberg, E.; Lonsdale, C. J.; 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.; Shankar, N. Udaya; Srivani, K. S.; Stevens, J.; Subrahmanyan, R.; Tingay, S. J.; Wayth, R. B.; Waterson, M.; Webster, R. L.; Whitney, A. R.; Williams, A.; Williams, C. L.; Wyithe, J. S. B.en
dc.identifier.orcidhttps://orcid.org/0000-0002-4117-570X
dc.identifier.orcidhttps://orcid.org/0000-0001-7130-208X
mit.licenseOPEN_ACCESS_POLICYen_US
mit.metadata.statusComplete


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