  The DANCe survey provides photometric and astrometric (position and proper
motion) measurements for approximately 2 millions unique sources in a region
encompassing $\approx$80deg$^{2}$ centered around the Pleiades cluster.
  We aim at deriving a complete census of the Pleiades, and measure the mass
and luminosity function of the cluster. Using the probabilistic selection
method described in Sarro+2014, we identify high probability members in the
DANCe ($i\ge$14mag) and Tycho-2 ($V\lesssim$12mag) catalogues, and study the
properties of the cluster over the corresponding luminosity range. We find a
total of 2109 high probability members, of which 812 are new, making it the
most extensive and complete census of the cluster to date. The luminosity and
mass functions of the cluster are computed from the most massive members down
to $\approx$0.025M$_{\odot}$. The size, sensitivity and quality of the sample
result in the most precise luminosity and mass functions observed to date for a
cluster. Our census supersedes previous studies of the Pleiades cluster
populations, both in terms of sensitivity and accuracy.
