High-significance Sunyaev-Zel'dovich measurement:: Abell 1914 seen with the Arcminute Microkelvin Imager

被引:16
作者
Barker, Robert
Biddulph, Phillip
Bly, Dennis
Boysen, Roger
Brown, Anthony
Clementson, Christopher
Crofts, Michael
Culverhouse, Thomas
Czeres, Jaroslaw
Dace, Roger
D'Alessandro, Robert
Doherty, Peter
Duffett-Smith, Peter
Duggan, Kenneth
Ely, John
Felvus, Mike
Flynn, William
Geisbusch, Jorn
Grainge, Keith
Grainger, William
Hammet, David
Hills, Richard
Hobson, Michael
Holler, Christian
Jilley, Roy
Jones, Michael E.
Kaneko, Takeshi
Kneissl, Rudiger
Lancaster, Katy
Lasenby, Anthony
Marshall, Phil
Newton, Francis
Norris, Oliver
Northrop, Ian
Pooley, Guy
Quy, Vic
Saunders, Richard D. E.
Scaife, Anna
Schofield, Jack
Scott, Paul
Shaw, Clive
Taylor, Angela C.
Titterington, David
Velic, Marko
Waldram, Elizabeth
West, Simon
Wood, Brian
Yassin, Ghassan
Zwart, Jonathan
机构
[1] Cavendish Lab, Astrophys Grp, Cambridge CB3 0HE, England
[2] Columbia Univ, Dept Phys, New York, NY 10027 USA
[3] Univ Calif Berkeley, Dept Astron, Berkeley, CA 94720 USA
[4] Univ Calif Berkeley, Dept Phys, Berkeley, CA 94720 USA
[5] HH Wills Phys Lab, Astrophys Grp, Bristol, England
[6] Kavli Inst Particle Astrophys & Cosmol, Stanford, CA USA
基金
英国科学技术设施理事会;
关键词
galaxies : clusters : individual : A1914; cosmic microwave background;
D O I
10.1111/j.1745-3933.2006.00151.x
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We report the first detection of a Sunyaev - Zel'dovich (S - Z) decrement using the Arcminute Microkelvin Imager ( AMI). We have made commissioning observations towards the cluster of galaxies A1914 and detected the S - Z effect with a significance of 17 sigma in a uv-tapered map at a mean frequency of 15.75 GHz. The integrated S - Z flux density of - 8.6 +/- 0.5 mJy is consistent with a simple X-ray derived model for the intracluster gas. We find that the spectrum of the decrement, measured in the six channels between 13.5 - 18 GHz, fits well to that expected for the S - Z effect. The sensitivity of the telescope is consistent with the figures used in our simulations of cluster surveys with AMI.
引用
收藏
页码:L1 / L4
页数:4
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