Fig. 9.
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Distribution of Y5R500 with respect to Θs for the gNFW pressure model fits to Planck data (grey) in Planck Collaboration XVIII (2015) and to the NIKA2 + R18 + XMM-Newton data (blue) in this work. Different contours show the 68%, 95%, and 99% confidence intervals. The black star corresponds to the intersection between the Planck Collaboration XVIII (2015) distribution and the X-ray scaling law shown in Fig. 16 in Planck Collaboration XVIII (2015).
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