Batch discovery of nine z∼ 1 clusters using X-ray and K or R, z' images

We present the results of an initial search for clusters of galaxies at z ～ 1 and above, using data from 2.9 square degrees of XMM–Newton images. By selecting weak potentially extended X-ray sources with faint or no identifications in deep, ground-based optical imaging, we have constructed a starting sample of 19 high-redshift cluster candidates. Near-IR and R , z ' imaging of these fields identified nine of them as high-redshift systems. Six of these were confirmed spectroscopically, three at z ～ 1.0 and the other three in the  0.8 < z < 0.92  range. The remaining three systems have solid photometric evidence to be at   z _phot～ 0.8, 1.0  and 1.3. The present sample significantly increases the number of such clusters. The measured density of z ? 1 clusters, after discarding 'low'-redshift systems at z ? 0.92 is about 1.7 deg^?2 (with 68 per cent confidence interval equal to 1.0, 2.9]) for   f_X ? 2.5  10^?15 erg cm^?2 s^?1  (0.5–2] keV) and this is a lower limit, having screened not all potential z ～ 1 candidate clusters. Coordinates, X-ray measures and evidence for nine X-ray-selected high-redshift clusters is given.