1 INTRODUCTION

2 SDSS-III/BOSS CMASS SAMPLE

3 BIG MULTI DARK SIMULATION

4 METHODOLOGY: THE SURVEY GENERATOR CODE
4.1 Halo Abundance Matching procedure
4.2 Stellar Mass Function
4.3 Production of Light-cones
4.4 Stellar Mass Incompleteness
4.5 Fiber Collisions

5 MODELLING BOSS CMASS CLUSTERING
5.1 Two point clustering: result from model and observations
5.2 Three-point correlation function
5.3 Stellar to halo mass relation
5.4 Bias prediction

6 DISCUSSION

7 SUMMARY