SZ/X-ray scaling relations using X-ray data and Planck Nominal maps

Abstract

We determine the relation between the Comptonization parameter predicted using X-ray data $Y_{C,Xray}$ and the X-ray luminosity $L_X$, both magnitudes derived from ROSAT data, with the Comptonization parameter $Y_{C,SZ}$ measured on {\it Planck} 2013 foreground cleaned Nominal maps. The 560 clusters of our sample includes clusters with masses $M\ge 10^{13}{M}_{\odot }$, one order of magnitude smaller than those used by the Planck Collaboration in a similar analysis. It also contains eight times more clusters in the redshift interval $z\le 0.3$. The prediction of the $\beta =2/3$ model convolved with the Planck antenna beam agrees with the anisotropies measured in foreground cleaned Planck Nominal maps within the X-ray emitting region, confirming the results of an earlier analysis (Atrio-Barandela et al. 2008). The universal pressure profile overestimates the signal by a 15-21\% depending on the angular aperture. We show that the discrepancy is not due to the presence of {\it cool-core} systems but it is an indication of a brake in the $L_X-M$ relation towards low mass systems. We show that relation of the Comptonization parameter averaged over the region that emits 99\% of the X-ray flux and and the X-ray luminosity is consistent with the predictions of the self-similar model. We confirm previous findings that the scaling relations studied here do not evolve with redshift within the range probed by our catalog.

13 pages, 5 figures, 3 tables. Accepted for publication in MNRAS

References in corpus (12)

• Some Aspects of Measurement Error in Linear Regression of Astronomical Data
• Statistics of X-ray observables for the cooling-core and non-cooling core galaxy clusters
• The Representative XMM-Newton Cluster Structure Survey (REXCESS) of an X-ray Luminosity Selected Galaxy Cluster Sample
• Scaling Properties of a Complete X-ray Selected Galaxy Group Sample
• Calibration of the galaxy cluster M_500-Y_X relation with XMM-Newton
• The Lx-Yx Relation: Using Galaxy Cluster X-Ray Luminosity as a Robust, Low Scatter Mass Proxy
• The X-Ray Luminosity--Mass Relation for Local Clusters of Galaxies
• LoCuSS: A Comparison of Sunyaev-Zel'dovich Effect and Gravitational Lensing Measurements of Galaxy Clusters
• Galaxy Cluster Scaling Relations between Bolocam Sunyaev-Zel'dovich Effect and Chandra X-ray Measurements
• The Impact of Galaxy Cluster Mergers on Cosmological Parameter Estimation from Surveys of the Sunyaev-Zel'dovich Effect
• Measurement of the electron-pressure profile of galaxy clusters in Wilkinson Microwave Anisotropy Probe (WMAP) 3-year data
• Analysis of Sunyaev-Zel'dovich Effect Mass-Observable Relations using South Pole Telescope Observations of an X-ray Selected Sample of Low Mass Galaxy Clusters and Groups

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• Free-form modelling of galaxy clusters: a Bayesian and data-driven approach
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