Robustness to the choice of mass function. The grey shaded contours give the cosmological constraints when using the Tinker et al. (2008) mass function, corresponding to our final result. This is compared to constraints obtained when using the Watson et al. (2013a) mass function, shown as the red shaded contours. In this figure we adopt the SZ+BAO+BBN data set and the CCCP mass bias prior.
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