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The Murchison Widefield Array

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arxiv 1008.2551 v1 pith:FJ4BX62C submitted 2010-08-15 astro-ph.IM

Daniel A. Mitchell , Lincoln J. Greenhill , Stephen M. Ord , Gianni Bernardi , Randall B. Wayth , Richard G. Edgar , Michael A. Clark , Kevin Dal
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Hanspeter Pfister Stewart J. Gleadow W. Arcus F.H. Briggs L. Benkevitch J.D. Bowman J.D. Bunton S. Burns R.J. Cappallo B.E. Corey A. de Oliveira-Costa L. Desouza S.S. Doeleman M.F. Derome D. Emrich M. Glossop R. Goeke M.R. Gopala Krishna B. Hazelton D.E. Herne J.N. Hewitt P.A. Kamini D.L. Kaplan J.C. Kasper B.B. Kincaid J. Kocz E. Kowald E. Kratzenberg D. Kumar C.J. Lonsdale M.J. Lynch S. Madhavi M. Matejek S.R. McWhirter M.F. Morales E. Morgan D. Oberoi J. Pathikulangara T. Prabu A. Rogers J.E. Salah R.J. Sault N. Udaya Shankar K.S. Srivani J. Stevens S.J. Tingay A. Vaccarella M. Waterson R.L. Webster A.R. Whitney A. Williams C. Williams
This is my paper · ORCID
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keywords murchisonarraywidefieldallowsautonomouslybandblankingcalibrate
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It is shown that the excellent Murchison Radio-astronomy Observatory site allows the Murchison Widefield Array to employ a simple RFI blanking scheme and still calibrate visibilities and form images in the FM radio band. The techniques described are running autonomously in our calibration and imaging software, which is currently being used to process an FM-band survey of the entire southern sky.

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