Measuring the growth of structure by matching dark matter haloes to
  galaxies with VIPERS and SDSS
  We test the history of structure formation from redshift 1 to today by
matching galaxies from VIPERS and SDSS with dark matter haloes in the MultiDark
SMDPL N-body simulation. We first show that the standard subhalo abundance
matching (SHAM) recipe implemented with MultiDark characterizes the clustering
of galaxies well both at redshift 0 for SDSS and at redshift 1 for VIPERS. This
is an important validation of the SHAM model at high redshift. We then remap
the simulation timesteps to test alternative growth histories and infer the
growth index $\gamma=0.6\pm0.3$. This analysis demonstrates the power of using
N-body simulations to forward model galaxy surveys for cosmological inference.
