Using SuZIE arcminute-scale CMB anisotropy data to probe open and flat-\Lambda CDM cosmogonies

A.E. Lange; Bharat Ratra; K. Ganga; Naoshi Sugiyama; P.A.R. Ade; P.D. Mauskopf; S.E. Church; W.L. Holzapfel

arxiv: astro-ph/9702186 · v1 · submitted 1997-02-21 · 🌌 astro-ph

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

K. Ganga , Bharat Ratra , S.E. Church , Naoshi Sugiyama , P.A.R. Ade , W.L. Holzapfel , A.E. Lange , P.D. Mauskopf This is my paper

classification 🌌 astro-ph

keywords anisotropyarcminute-scalecosmogoniesdataexperimentlimitsopenamplitude

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We 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.

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

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