1 INTRODUCTION

2 METHOD
2.1 Sample-variance cancellation simulations
2.2 Quasi N-body simulation
2.3 Calculating power spectra
2.4 Mock halo/galaxy samples in comparison to future survey targets
2.5 Estimating power spectrum covariance matrix
2.6 Density field reconstruction
2.7 Fitting models
2.8 MCMC fitting

3 RESULTS
3.1 BAO scales in matter distribution
3.2 BAO scales in the presence of galaxy/halo bias
3.3 BAO systematics dependence on reconstruction conventions
3.4 Nonlinear damping scales
3.5 Redshift-space distortion parameter–growth rate f
3.6 Nonlinear scale-dependent bias b∂
3.7 Shot noise dependence
3.8 Smoothing scale Σsm dependence
3.9 Parameter covariances

4 CONCLUSION