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Using Sunyaev-Zeldovich infrared experiment (SuZIE) arcminute-scale cosmic microwave background anisotropy data to probe open and flat Lambda cold dark matter cosmogonies

被引：21
作者：
Ganga, K
Ratra, B
Church, SE
Sugiyama, N
Ade, PAR
Holzapfel, WL
Mauskopf, PD
Lange, AE
机构：
[1] CALTECH, DIV PHYS MATH & ASTRON, PASADENA, CA 91125 USA
[2] MIT, CTR THEORET PHYS, CAMBRIDGE, MA 02139 USA
[3] KYOTO UNIV, DEPT PHYS, SAKYO KU, KYOTO 606, JAPAN
[4] UNIV LONDON QUEEN MARY & WESTFIELD COLL, DEPT PHYS, LONDON E1 4NS, ENGLAND
来源：
ASTROPHYSICAL JOURNAL | 1997年 / 484卷 / 02期
关键词：
cosmic microwave background; cosmology; observations; large-scale structure of universe;
D O I：
10.1086/304365
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We use arcminute-scale data from the Sunyaev-Zeldovich Infrared Experiment to set limits on anisotropies in cosmic microwave background radiation in open and spatially flat A 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 Differential Microwave Radiometer experiment.
引用
收藏
页码：517 / 522
页数：6
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