Using White Dish CMB Anisotropy Data to Probe Open and Flat-Lambda CDM Cosmogonies

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dc.creatorRatra, B.
dc.creatorGanga, K.
dc.creatorSugiyama, N.
dc.creatorTucker, G. S.
dc.creatorGriffin, G. S.
dc.creatorNguyen, H. T.
dc.creatorPeterson, J. B.
dc.date1997-10-24
dc.date.accessioned2026-07-07T11:34:07Z
dc.date.available2026-07-07T11:34:07Z
dc.descriptionWe use data from the White Dish experiment to set limits on cosmic microwave background radiation anisotropies in open and spatially-flat-Lambda cold dark matter cosmogonies. We account for the White Dish calibration uncertainty, and marginalize over the offset and gradient removed from the data. Our 2-sigma upper limits are larger than those derived previously. These upper limits are consistent with those derived from the $COBE$-DMR data for all models tested.
dc.description17 pages of latex. Uses aasms4.sty. 4 figures included. Submitted to ApJS
dc.identifierhttps://arxiv.org/abs/astro-ph/9710270
dc.identifierhttp://arxiv.org/abs/astro-ph/9710270
dc.identifierAstrophys.J.505:8-11,1998
dc.identifierdoi:10.1086/306139
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/198131
dc.subjectAstrophysics
dc.titleUsing White Dish CMB Anisotropy Data to Probe Open and Flat-Lambda CDM Cosmogonies
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