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Sunyaev-Zel'dovich observations with AMI of the hottest galaxy clusters detected in the XMM-Newton Cluster Survey

Authors :
Farhan Feroz
Michel P. Schammel
Anthony Lasenby
Clare Rumsey
Natasha Hurley-Walker
Michael P. Hobson
A. Kathy Romer
David Titterington
Elizabeth Waldram
Anna M. M. Scaife
Yvette C. Perrott
Keith Grainge
Malak Olamaie
Paul F. Scott
E. J. Lloyd-Davies
C. Rodriguez-Gonzalvez
Thomas M. O. Franzen
Richard D. E. Saunders
Guy G. Pooley
Source :
Monthly Notices of the Royal Astronomical Society. 433:2920-2937
Publication Year :
2013
Publisher :
Oxford University Press (OUP), 2013.

Abstract

We have obtained deep Sunyaev–Zel’dovich (SZ) observations towards 15 of the hottest XMM Cluster Survey (XCS) clusters that can be observed with the Arcminute Microkelvin Imager (AMI). We use a Bayesian analysis to quantify the significance of our SZ detections. We detect the SZ effect at high significance towards three of the clusters and at lower significance for a further two clusters. Towards the remaining 10 clusters, no clear SZ signal was measured. We derive cluster parameters using the XCS mass estimates as a prior in our Bayesian analysis. For all AMI-detected clusters, we calculate large-scale mass and temperature estimates while for all undetected clusters we determine upper limits on these parameters. We find that the large-scale mean temperatures derived from our AMI SZ measurements (and the upper limits from null detections) are substantially lower than the XCS-based core-temperature estimates. For clusters detected in the SZ, the mean temperature is, on average, a factor of 1.4 lower than temperatures from the XCS. Our upper limits on the cluster temperature of undetected systems are lower than the mean XCS derived temperature.

Details

ISSN :
13652966 and 00358711
Volume :
433
Database :
OpenAIRE
Journal :
Monthly Notices of the Royal Astronomical Society
Accession number :
edsair.doi.dedup.....cd462c13a84ed467afb912178b5c4876
Full Text :
https://doi.org/10.1093/mnras/stt932