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We present a list of 15 clusters of galaxies, serendipitously detected by the  XMM  Cluster Survey (XCS), that have a high probability of detection by the  Planck  satellite. Three of them already appear in the  Planck  Early Sunyaev–Zel’dovich (ESZ) catalogue. The estimation of the  Planck  detection probability assumes the flat Lambda cold dark matter (ΛCDM) cosmology most compatible with 7‐year  Wilkinson Microwave Anisotropy Probe  ( WMAP 7) data. It takes into account the XCS selection function and  Planck  sensitivity, as well as the covariance of the cluster X‐ray luminosity, temperature and integrated Comptonization parameter, as a function of cluster mass and redshift, determined by the Millennium gas simulations. We also characterize the properties of the galaxy clusters in the final data release of the XCS that we expect  Planck  will have detected by the end of its extended mission. Finally, we briefly discuss possible joint applications of the XCS and  Planck  data.

The XMM Cluster Survey: predicted overlap with the Planck Cluster Catalogue