SZ science with an ALMA band 1 receiver system

被引：0

作者：

Scaife, Anna M. M. ^{[1
]}

Grainge, Keith J. B. ^{[2
,3
]}

机构：

[1] Dublin Inst Adv Studies, Dublin 2, Ireland

[2] Univ Cambridge, Cavendish Lab, Astrophys Grp, Cambridge CB3 0HE, England

[3] Kavli Inst Cosmol, Cambridge, England

来源：

BULLETIN OF THE ASTRONOMICAL SOCIETY OF INDIA | 2010年 / 38卷 / 04期

关键词：

instrumentation: interferometers; radiation mechanisms: general; galaxies: clusters; CLUSTERS; PLASMA; GAS;

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present the first full interferometric simulations of galaxy clusters containing radio plasma bubbles as observed by the proposed Q band receiver system for the ALMA telescope. We discuss the observational requirements for detecting intracluster substructure directly from the SZ signal and the advantages of these observations over those made with the current generation of SZ survey instruments.

引用

页码：185 / 193

页数：9

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