BIMA observations of possible microwave background sources

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dc.creatorChernin, Lawrence M.
dc.creatorScott, Douglas
dc.date1994-08-05
dc.date.accessioned2026-07-07T02:19:21Z
dc.date.available2026-07-07T02:19:21Z
dc.descriptionWe present sensitive upper limits on the 90 GHz flux of known radio and infrared sources in regions associated with possible cosmic microwave background fluctuations at 0.5--1 degree scales. Specifically we look at the MAX GUM region and the region of strongest fluctuation in the MSAM scan. None of the known sources can account for the levels of anisotropy seen.
dc.description2 pages, postscript, CfPA-94-37
dc.identifierhttps://arxiv.org/abs/astro-ph/9408021
dc.identifierhttp://arxiv.org/abs/astro-ph/9408021
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/9828
dc.subjectAstrophysics
dc.titleBIMA observations of possible microwave background sources
dc.typetext

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