Distant galaxy clusters in the XMM Large Scale Structure survey
  (Abridged) Distant galaxy clusters provide important tests of the growth of
large scale structure in addition to highlighting the process of galaxy
evolution in a consistently defined environment at large look back time. We
present a sample of 22 distant (z>0.8) galaxy clusters and cluster candidates
selected from the 9 deg2 footprint of the overlapping X-ray Multi Mirror (XMM)
Large Scale Structure (LSS), CFHTLS Wide and Spitzer SWIRE surveys. Clusters
are selected as extended X-ray sources with an accompanying overdensity of
galaxies displaying optical to mid-infrared photometry consistent with z>0.8.
Nine clusters have confirmed spectroscopic redshifts in the interval 0.8<z<1.2,
four of which are presented here for the first time. A further 11 candidate
clusters have between 8 and 10 band photometric redshifts in the interval
0.8<z<2.2, while the remaining two candidates do not have information in
sufficient wavebands to generate a reliable photometric redshift. All of the
candidate clusters reported in this paper are presented for the first time.
Those confirmed and candidate clusters with available near infrared photometry
display evidence for a red sequence galaxy population, determined either
individually or via a stacking analysis, whose colour is consistent with the
expectation of an old, coeval stellar population observed at the cluster
redshift. We further note that the sample displays a large range of red
fraction values indicating that the clusters may be at different stages of red
sequence assembly. We compare the observed X-ray emission to the flux expected
from a suite of model clusters and find that the sample displays an effective
mass limit M200 ~ 1e14 Msolar with all clusters displaying masses consistent
with M200 < 5e14 Msolar. This XMM distant cluster study represents a complete
sample of X-ray selected z>0.8 clusters.
