Planck Early Results. X. Statistical analysis of Sunyaev-Zeldovich scaling relations for X-ray galaxy clusters
Planck Collaboration: N. Aghanim, M. Arnaud, M. Ashdown, J. Aumont, C., Baccigalupi, A. Balbi, A. J. Banday, R. B. Barreiro, M. Bartelmann, J. G., Bartlett, E. Battaner, K. Benabed, A. Beno\^it, J.-P. Bernard, M. Bersanelli,, R. Bhatia, J. J. Bock, A. Bonaldi, J. R. Bond

TL;DR
This study combines Planck and X-ray data to analyze the Sunyaev-Zeldovich effect in galaxy clusters, confirming the scaling relations and their evolution with high significance and no evidence of deviation from standard models.
Contribution
It provides the first measurement of the intrinsic scatter in SZ-X-ray luminosity scaling relations and confirms the consistency of SZ and X-ray observations across a wide luminosity range.
Findings
High-significance detection of SZ signal across luminosity range
Excellent agreement between Planck measurements and X-ray predictions
No evidence of deviation from standard scaling relation evolution
Abstract
All-sky data from the Planck survey and the Meta-Catalogue of X-ray detected Clusters of galaxies (MCXC) are combined to investigate the relationship between the thermal Sunyaev-Zeldovich (SZ) signal and X-ray luminosity. The sample comprises ~ 1600 X-ray clusters with redshifts up to ~ 1 and spans a wide range in X-ray luminosity. The SZ signal is extracted for each object individually, and the statistical significance of the measurement is maximised by averaging the SZ signal in bins of X-ray luminosity, total mass, or redshift. The SZ signal is detected at very high significance over more than two decades in X-ray luminosity (10^43 erg/s < L_500 E(z)^-7/3 < 2 X 10^45 erg/s). The relation between intrinsic SZ signal and X-ray luminosity is investigated and the measured SZ signal is compared to values predicted from X-ray data. Planck measurements and X-ray based predictions are found…
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