  We present the statistical methods that have been developed to analyse the
OzDES reverberation mapping sample. To perform this statistical analysis we
have created a suite of customisable simulations that mimic the characteristics
of each individual source in the OzDES sample.These characteristics include:
the variability in the photometric and spectroscopic lightcurves,the
measurement uncertainties and the observational cadence. By simulating six real
sources that contain the CIV emission line, we developed a set of quality
criteria that ranks the reliability of a recovered time lag depending on the
agreement between different recovery methods, the magnitude of the
uncertainties, and the rate at which false positives were found in the
simulations. Of these six sources, two were given a quality rating of 1,
corresponding to our 'gold standard'. Lags were recovered at 223$\pm$56 and
378$\pm$104 days with redshifts of 1.93 and 2.74 respectively. Future work will
apply these methods to the entire OzDES sample of $\sim$750 AGN.
