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We update the cosmological parameter estimation for three non-vanilla modelsby a joint analysis of \CCCP\ X-ray cluster, the newly released \Planck\ CMBdata as well as some external data sets, such as baryon acoustic oscillationmeasurements from the 6dFGS, SDSS DR7 and BOSS DR9 surveys, and Hubble SpaceTelescope $H_0$ measurement. First of all, we find that X-ray cluster data setsstrongly favor a non-zero summed neutrino mass at more than 3$\sigma$confidence level in these non-vanilla models. And then, we reveal some tensionsbetween X-ray cluster and {\it Planck} data in some cosmological parameters.For the matter power spectrum amplitude $\sigma_8$, X-ray cluster data favor alower value compared with {\it Planck}. Because of the strong $\sigma_8-\summ_{\nu}$ degeneracy, this tension could beyond 2$\sigma$ confidence level whenthe summed neutrino mass $\sum m_{\nu}$ is allowed to vary. For the CMB lensingamplitude $A_L$, the addition of X-ray cluster data results in a 3$\sigma$deviation from the vanilla model. Furthermore, {\it Planck}+X-ray data prefer alarge Hubble constant and phantom-like dark energy equation of state, which arein $2\sigma$ tension with those from WMAP7+X-ray data. Finally, we find thatthese tensions/descrepencies could be relaxed in some sense by adding a $9\%$systematic shift in the cluster mass functions.

Cosmological parameter estimation from CMB and X-ray clusters after Planck