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Limits on Hot Intracluster Gas Contributions to the Tenerife Temperature Anisotropy Map

机译:特内里费岛温度各向异性图对集群内热气体贡献的限制

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摘要

We limit the contribution of the hot intracluster gas, by means of theSunyaev-Zel'dovich effect, to the temperature anisotropies measured by theTenerife experiment. The data is cross-correlated with maps generated from theACO cluster catalogue, the ROSAT PSPC catalogue of clusters of galaxies, acatalogue of superclusters and the HEAO 1 A-1 map of X-ray sources. There is noevidence of contamination by such sources at an rms level of $\sim 8\mu$K at99onfidence level at $5^o$ angular resolution. We place an upper limit onthe mean Comptonization parameter of $ y \le 1.5\times 10^{-6}$ at the samelevel of confidence. These limits are slightly more restrictive than thosepreviously found by a similar analysis on the COBE/DMR data and indicate thatmost of the signal measured by Tenerife is cosmological.
机译:通过Sunyaev-Zel'dovich效应,我们限制了集群内热气体对通过Tenerife实验测得的温度各向异性的贡献。该数据与从ACO团簇目录,星系团簇的ROSAT PSPC目录,超级团簇目录和X射线源HEAO 1 A-1谱图生成的图谱互相关。没有证据表明在角分辨率为$ 5 ^ o的均方根值(rms)为\\ sim 8 \ mu $ K的情况下,此类源会造成污染。我们在相同置信度下对$ y \ le 1.5 \乘以10 ^ {-6} $的平均Comptonization参数设置了上限。这些限制比以前对COBE / DMR数据进行的类似分析所发现的限制要严格一些,这表明特内里费岛测得的大多数信号都是宇宙学的。

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