Using SuZIE arcminute-scale CMB anisotropy data to probe open and flat-ΛCDM cosmogonies

Simple item page
dc.creatorGanga, K.
dc.creatorRatra, Bharat
dc.creatorChurch, S. E.
dc.creatorSugiyama, Naoshi
dc.creatorAde, P. A. R.
dc.creatorHolzapfel, W. L.
dc.creatorLange, A. E.
dc.creatorMauskopf, P. D.
dc.date1997-02-21
dc.date.accessioned2026-07-07T11:34:06Z
dc.date.available2026-07-07T11:34:06Z
dc.descriptionWe use arcminute-scale data from the Sunyaev-Zel'dovich Infrared Experiment to set limits on anisotropies in the cosmic microwave background radiation in open and spatially-flat-Lambda cold dark matter cosmogonies. There are no 2-sigma detections for the models tested. The upper limits obtained are consistent with the amplitude of anisotropy detected by the COBE/DMR experiment.
dc.description17 pages including 4 postscript figures. Latex. Uses aaspp4. ApJ, in press
dc.identifierhttps://arxiv.org/abs/astro-ph/9702186
dc.identifierhttp://arxiv.org/abs/astro-ph/9702186
dc.identifierAstrophys.J.484:517-522,1997
dc.identifierdoi:10.1086/304365
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/198124
dc.subjectAstrophysics
dc.titleUsing SuZIE arcminute-scale CMB anisotropy data to probe open and flat-ΛCDM cosmogonies
dc.typetext

Files

Collections

arXiv