Cosmological constraints from the Planck cluster catalogue with new multi-wavelength mass calibration from Chandra and CFHT

Open Access

Fig. 7

Calibration of the $Y_{SZ} - M_{500}^{Y_{X}}$ $\[Y_{\mathrm{SZ}}-M_{500}^{Y_{\mathrm{X}}}\]$ scaling relation for the high (best fit in red) and low (best fit in green) redshift subsamples. The black line shows the best-fit relation obtained previously on the full sample, and the grey contours correspond to 1σ uncertainties for each subsample fit.

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