The YSZ,Planck - YSZ,XMM scaling relation and its difference between cool-core and non-cool-core clusters

Abstract

We construct a sample of 70 clusters using data from XMM-Newton and Planck to investigate the Y SZ,Planck-Y SZ, XMM scaling relation and the cool-core influences on the relation. Y SZ,XMM is calculated by accurate de-projected temperature and electron number density profiles derived from XMM-Newton. Y SZ,Planck is the latest Planck data restricted to our precise X-ray size θ 500. To study the cool-core influences onY SZ,Planck-Y SZ, XMM scaling relation, we apply two criteria, limits of central cooling time and classic mass deposition rate, to distinguish cool-core clusters (CCCs) from non-cool-core clusters (NCCCs). We also use Y SZ,Planck from other papers, which are derived from different methods, to confirm our results. The intercept and slope of theY SZ,Planck-Y SZ, XMM scaling relation are A=-0.86 0.30, B=0.83 0.06. The intrinsic scatter is σ ins= 0.14 0.03. The ratio of Y SZ,Planck/Y SZ, XMM is 1.03 0.05, which is perfectly agreed with unity. Discrepancies of Y SZ,Planck-Y SZ, XMM scaling relation between CCCs and NCCCs are found in observation. They are independent of cool-core classification criteria and Y SZ,Planck calculation methods, although discrepancies are more significant under the classification criteria of classic mass deposition rate. The intrinsic scatter of CCCs (0.04) is quite small compared to that of NCCCs (0.27). The ratio of Y SZ,Planck/Y SZ, XMM for CCCs is 0.89 0.05, suggesting that CCCs' Y SZ,XMM may overestimate SZ signal. By contrast, the ratio of Y SZ,Planck/Y SZ, XMM for NCCCs is 1.14 0.12, which indicates that NCCCs' Y SZ,XMM may underestimate SZ signal.

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