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Andrade-Santos, Felipe; Pratt, Gabriel W.; Melin, Jean-Baptiste; Arnaud, Monique; Jones, Christine; Forman, William R.; Pointecouteau, Etienne; Bartalucci, Iacopo; Vikhlinin, Alexey; Murray, Stephen S.; Mazzotta, Pasquale; Borgani, Stefano; Lovisari, Lorenzo; van Weeren, Reinout J.; Kraft, Ralph P.; David, Laurence P.; Giacintucci, Simona
Astrophysical journal/The Astrophysical journal, 06/2021, Volume: 914, Issue: 1Journal Article
Abstract Using Chandra observations, we derive the Y X proxy and associated total mass measurement, , for 147 clusters with z < 0.35 from the Planck early Sunyaev–Zeldovich catalog, and for 80 clusters with z < 0.22 from an X-ray flux-limited sample. We reextract the Planck Y SZ measurements and obtain the corresponding mass proxy, , from the full Planck mission maps, minimizing Malmquist bias due to observational scatter. The masses reextracted using the more precise X-ray position and characteristic size agree with the published PSZ2 values, but yield a significant reduction in the scatter (by a factor of two) in the – relation. The slope is 0.93 ± 0.03, and the median ratio, , is within the expectations from known X-ray calibration systematics. Y SZ / Y X is 0.88 ± 0.02, in good agreement with predictions from cluster structure, and implying a low level of clumpiness. In agreement with the findings of the Planck Collaboration, the slope of the Y SZ – flux relation is significantly less than unity (0.89 ± 0.01). Using extensive simulations, we show that this result is not due to selection effects, intrinsic scatter, or covariance between quantities. We demonstrate analytically that changing the Y SZ – Y X relation from apparent flux to intrinsic properties results in a best-fit slope that is closer to unity and increases the dispersion about the relation. The redistribution resulting from this transformation implies that the best-fit parameters of the – relation will be sample-dependent.
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