Foregrounds and experiments below 33GHz

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dc.creatorJones, A. W.
dc.date1999-05-07
dc.date.accessioned2026-07-07T02:31:31Z
dc.date.available2026-07-07T02:31:31Z
dc.descriptionIn this paper I report on the recent results obtained from the Tenerife switched beam (10 GHz to 33 GHz) experiment and Jodrell Bank 5 GHz interferometer and their predictions for foreground levels. The full data analysis and results will be presented elsewhere. It is found that free-free emission dominates above 10 GHz, whereas synchrotron emission dominates below 5 GHz.
dc.description7 pages, 5 figures, invited review in "Microwave Foregrounds", eds. A de Oliveira-Costa & M. Tegmark (ASP: San Francisco)
dc.identifierhttps://arxiv.org/abs/astro-ph/9905087
dc.identifierhttp://arxiv.org/abs/astro-ph/9905087
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/14182
dc.subjectAstrophysics
dc.titleForegrounds and experiments below 33GHz
dc.typetext

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