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The brightness and spatial distributions of terrestrial radio sources

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Offringa, Andre; Butcher, Harvey; de Bruyn, A. G.; Zaroubi, Saleem; Koopmans, L. V. E.; Wijnholds, S. J.; Abdalla, Filipe B.; Brouw, W. N.; Ciardi, Benedetta; Iliev, I. T.; Harker, Geraint; Mellema, G.; Bernardi, G.; Zarka, P.; Ghosh, A.; Alexov, A.; Anderson, J. M.; Asgekar, A.; Avruch, Ian M.; Bell, Michael R.; Bentum, M. J.; Breitling, F.; de Gasperin, F.; de Geus, Eugene; de Vos, Marco; Duscha, S.; Fallows, R. A.; Frieswijk, W.; Garrett, M. A.; Iacobelli, M.; Klijn, W.; Kondratiev, V. I.; Kuniyoshi, M.; Kuper, G.; van Leeuwen, J.; Maat, P.; Mann, Gottfried; McKean, J. P.; Norden, M. J.; Pizzo, R.; Polatidis, A. G.; Rafferty, D. A.; Reich, W.; Van Nieuwpoort, Rob; Sluman, J.; Sobey, C.; Tang, Y.; Toribio, C.; Vermeulen, R. C.; Vocks, Christian; Wise, M. J.

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Faint undetected sources of radio-frequency interference (RFI) might become visible in long radio observations when they are consistently present over time. Thereby, they might obstruct the detection of the weak astronomical signals of interest. This issu

CollectionsANU Research Publications
Date published: 2013
Type: Journal article
URI: http://hdl.handle.net/1885/75015
Source: Monthly Notices of the Royal Astronomical Society
DOI: 10.1093/mnras/stt1337
Access Rights: Open Access

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