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The 154 MHz radio sky observed by the Murchison Widefield Array: noise, confusion and first source count analyses

Franzen, T. M. O.; Jackson, C. A.; Offringa, Andre; Ekers, R. D.; Wayth, R. B.; Bernardi, G.; Bowman, J. D.; Briggs, F.; Cappallo, R. J.; Deshpande, A. A.; Gaensler, B. M.; Greenhill, L. J.; Hazelton, B. J.; Johnston-Hollitt, M.; Kaplan, D. L.; Lonsdale, C. J.; McWhirter, S. R.; Mitchell, D. A.; Morales, M. F.; Morgan, E.; Morgan, J.; Oberoi, D.; Ord, S. M.; Prabu, T.; Seymour, N.; Udaya Shankar, N.; Srivani, K. S.; Subrahmanyan, R.; Tingay, S. J.; Trott, C. M.; Webster, R. L.; Williams, A.; Williams, C. L.

Description

We analyse a 154 MHz image made from a 12 h observation with the Murchison Widefield Array (MWA) to determine the noise contribution and behaviour of the source counts down to 30 mJy. The MWA image has a bandwidth of 30.72 MHz, a field-of-view within the half-power contour of the primary beam of 570 deg², a resolution of 2.3 arcmin and contains 13 458 sources above 5σ. The rms noise in the centre of the image is 4-5 mJy beam⁻¹. The MWA counts are in excellent agreement with counts from other...[Show more]

CollectionsANU Research Publications
Date published: 2016-04-13
Type: Journal article
URI: http://hdl.handle.net/1885/107205
Source: Monthly Notices of the Royal Astronomical Society
DOI: 10.1093/mnras/stw823

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