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首页> 外文期刊>The Astrophysical journal >CROSS-CORELATION OF THE 2-10 keV X-RAY BACKGROUND WITH RADIO SOURCES: CONSTRAINING THE LARGE-SCALE STRUCTURE OF THE X-RAY BACKGROUND
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CROSS-CORELATION OF THE 2-10 keV X-RAY BACKGROUND WITH RADIO SOURCES: CONSTRAINING THE LARGE-SCALE STRUCTURE OF THE X-RAY BACKGROUND

机译:2-10 keV X射线背景与无线电源的互相关:约束X射线背景的大型结构

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摘要

We present cross-correlation analyses of the HEAO 2-10 keV diffuse X-ray map with both the com- bined GB6/Parkes-MIT-NRAO (GB6-PMN) 5 GHz and the FIRST 1.4 GHz radio surveys. The cross- correlation functions (CCFs) of both radio surveys with the unresolved X-ray background were detected at the 5 σ level. While the large angular resolution (3°) of the X-ray map makes it difficult to separate the contributions of clustering from those of Poisson fluctuations, the amplitude of the CCF provides important constraints on the X-ray emissivity of the radio sources, as well as on the clustering properties of radio and X-ray sources.
机译:我们将结合使用GB6 / Parkes-MIT-NRAO(GB6-PMN)5 GHz和FIRST 1.4 GHz无线电测量数据对HEAO 2-10 keV漫射X射线图进行互相关分析。在5σ水平上检测到两个无线电测量与X射线背景未分辨的互相关函数(CCF)。尽管X射线图的大角度分辨率(3°)使得很难将聚类的贡献与泊松涨落的贡献分开,但CCF的幅度对无线电源的X射线发射率提供了重要的限制,因为以及无线电和X射线源的聚类属性。

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