Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/6493
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dc.contributor.authorFranzen, Thomas M.O.-
dc.contributor.authorJackson, C.A-
dc.contributor.authorDwarakanath, K.S.-
dc.contributor.authorOffringa, A.R.-
dc.contributor.author+20 Co-authors-
dc.date.accessioned2016-11-22T13:42:25Z-
dc.date.available2016-11-22T13:42:25Z-
dc.date.issued2015-
dc.identifier.citationProceedings of Science from The many facets of extragalactic radio surveys: towards new scientific challenges (EXTRA-RAD SUR2015). 20-23 October 2015, held at Bologna, Italy, Page - 53en_US
dc.identifier.issn1824-8039.-
dc.identifier.urihttp://hdl.handle.net/2289/6493-
dc.descriptionOpen Accessen_US
dc.description.abstractThe GaLactic and Extragalactic All-sky MWA survey (GLEAM) is a new relatively low resolution, contiguous 72–231 MHz survey of the entire sky south of declination +25◦. In this paper, we outline one approach to determine the relative contribution of system noise, classical confusion and sidelobe confusion in GLEAM images. An understanding of the noise and confusion properties of GLEAM is essential if we are to fully exploit GLEAM data and improve the design of future low-frequency surveys. Our early results indicate that sidelobe confusion dominates over the entire frequency range, implying that enhancements in data processing have the potential to further reduce the noiseen_US
dc.language.isoenen_US
dc.publisherSISSA, The International School for Advanced Studies, Trieste,en_US
dc.relation.urihttp://adsabs.harvard.edu/abs/2015mfer.confE..53Fen_US
dc.relation.urihttp://arxiv.org/abs/1604.04447en_US
dc.rights2015 The authors & the Royal Astronomical Societyen_US
dc.titleLimits of noise and confusion in the MWA GLEAM year 1 surveyen_US
dc.typeArticleen_US
Appears in Collections:Research Papers (A&A)

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