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dc.contributor.author | Grobler, Trienko Lups | |
dc.contributor.author | Nunhokee, C.D. | |
dc.contributor.author | Smirnov, Oleg M. | |
dc.contributor.author | Van Zyl, A.J. | |
dc.contributor.author | De Bruyn, A.G. | |
dc.date.accessioned | 2014-08-05T08:43:00Z | |
dc.date.available | 2014-08-05T08:43:00Z | |
dc.date.issued | 2014-04 | |
dc.description.abstract | This work investigates a particular class of artefacts, or ghost sources, in radio in- terferometric images. Earlier observations with (and simulations of) the Westerbork Synthesis Radio Telescope (WSRT) suggested that these were due to calibration with incomplete sky models. A theoretical framework is derived that validates this sug- gestion, and provides predictions of ghost formation in a two-source scenario. The predictions are found to accurately match the result of simulations, and qualitatively reproduce the ghosts previously seen in observational data. The theory also provides explanations for many previously puzzling features of these artefacts (regular geom- etry, PSF-like sidelobes, seeming independence on model ux), and shows that the observed phenomenon of ux suppression a ecting unmodelled sources is due to the same mechanism. We demonstrate that this ghost formation mechanism is a funda- mental feature of calibration, and exhibits a particularly strong and localized signature due to array redundancy. To some extent this mechanism will a ect all observations (including those with non-redundant arrays), though in most cases the ghosts remain hidden below the noise or masked by other instrumental artefacts. The implications of such errors on future deep observations are discussed. | en_US |
dc.description.librarian | hb2014 | en_US |
dc.description.sponsorship | South African Research Chairs Initiative of the Department of Science and Technology and National Research Foundation | en_US |
dc.description.uri | http://mnras.oxfordjournals.org | en_US |
dc.identifier.citation | Grobler, TL, Nunhokee, CD, Smirnov, OM, Van Zyl, AJ & De Bruyn, AG 2014, 'Calibration artefacts in radio interferometry - I. Ghost sources in Westerbork Synthesis Radio Telescope data', Monthly Notices of the Royal Astronomical Society, vol. 439, no. 4, pp. 4030-4047. | en_US |
dc.identifier.issn | 0035-8711(print) | |
dc.identifier.issn | 1365-2966 (online) | |
dc.identifier.other | 10.1093/mnras/stu268 | |
dc.identifier.uri | http://hdl.handle.net/2263/41074 | |
dc.language.iso | en | en_US |
dc.publisher | Oxford University Press | en_US |
dc.rights | © 2014 The Authors. All rights reserved.Oxford University Press. This is a pre-copy-editing, author-produced PDF of an article accepted for publication inc Monthly Notices of the Royal Astronomical Society vol. 439, no. 4, pp.4030-4047, 2014. doi : 10.1093/mnras/stu268. The definitive publisher-authenticated version is available online at : http://mnras.oxfordjournals.org. | en_US |
dc.subject | Instrumentation | en_US |
dc.subject | Interferometers | en_US |
dc.subject | Analytical methods | en_US |
dc.subject | Numerical techniques | en_US |
dc.subject | Radio interferometry | en_US |
dc.subject | Calibration artefacts | en_US |
dc.title | Calibration artefacts in radio interferometry - I. Ghost sources in Westerbork Synthesis Radio Telescope data | en_US |
dc.type | Postprint Article | en_US |