SIMBAD references

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 this relation. Y_SZ,XMM is calculated by accurately de-projected temperature and electron number density profiles derived from XMMNewton. Y_SZ,_Planck _is the latest Planck data restricted to our precise X-ray cluster size θ₅₀₀. To study the cool-core influences on the Y_SZ,Planck- Y_SZ,XMM scaling relation, we apply two criteria, namely the 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 the Y_SZ,Planck- Y_SZ,XMM scaling relation are A = -0.86±0.30 and B = 0.83±0.06 respectively. 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 in excellent statistical agreement with unity. Discrepancies in the Y_SZ,Planck- Y_SZ,XMM scaling relation between CCCs and NCCCs are found in the observation. They are independent of the cool-core classification criteria and Y_SZ,_Planck _calculation methods, although the 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 the Sunyaev-Zel'dovich (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 the SZ signal.