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Home All issues Volume 580 (August 2015) A&A, 580 (2015) A95 Online Material
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Issue
A&A
Volume 580, August 2015
Article Number A95
Number of page(s) 39
Section Cosmology (including clusters of galaxies)
DOI https://doi.org/10.1051/0004-6361/201424188
Published online 07 August 2015

Online material

Appendix A: Results table

Table A.1

Summary of results for all clusters between 20° ≤ δ< 87° with Planck S/N> 5.

Appendix B: Ytot–θs posterior comparison

thumbnail Fig. B.1

Ytot–θs posterior distributions for AMI and Planck, in descending Planck S/N order (note that this is the compatibility S/N for PwS), for all AMI detections (). Contours mark the 68% and 95% confidence limits of the posterior distributions. Where available, X-ray values for θs converted from θ500 values from Piffaretti et al. (2011) using the universal c500 = 1.177 are shown with black dotted lines.
Open with DEXTER

thumbnail Fig. B.1

continued.
Open with DEXTER

thumbnail Fig. B.1

continued.
Open with DEXTER

thumbnail Fig. B.1

continued.
Open with DEXTER

thumbnail Fig. B.1

continued.
Open with DEXTER

thumbnail Fig. B.1

continued.
Open with DEXTER

thumbnail Fig. B.1

continued.
Open with DEXTER

thumbnail Fig. B.1

continued.
Open with DEXTER

thumbnail Fig. B.1

continued.
Open with DEXTER

thumbnail Fig. B.2

Ytot–θs posterior distributions for AMI and Planck, in descending Planck S/N order (note that this is the compatibility S/N for PwS), for all AMI non-detections (). Contours mark the 68% and 95% confidence limits of the posterior distributions. Where available, X-ray values for θs converted from θ500 values from Piffaretti et al. (2011) using the universal c500 = 1.177 are shown with black dotted lines.
Open with DEXTER

thumbnail Fig. B.2

continued.
Open with DEXTER


© ESO, 2015

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