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

页码：517 / 522

页数：6

共 51 条

[21]

HOLZAPFEL WL, 1997, APJ, V479, P19

[22] A cosmic microwave background radiation measurement reproduced: A statistical comparison of MSAM1-94 to MSAM1-92 [J].