1. INTRODUCTION

2. DATA
2.1. Overview of the FMOS-COSMOS survey
2.2. Sample selection
2.3. Sample characteristics
2.4. Mock catalog

3. CORRECTIONS FOR CRITICAL BIASES
3.1. Fiber allocation
3.2. Integral constraint
3.3. Contamination by fake detection

4. RESULTS
4.1. Power-law model
4.2. Biased dark matter model
4.3. Comparisons of clustering strength

5. CONNECTION BETWEEN GALAXIES AND DARK MATTER HALOS
5.1. The halo model and occupation distribution
5.2. Limitations for the HOD parameters
5.3. HOD model fit

6. DISCUSSION
6.1. Halo mass and large-scale bias
6.2. Stellar mass-to-halo mass ratio
6.3. Baryon conversion efficiency
6.4. Satellite galaxies
6.5. Prediction for the future Subaru/PFS survey

7. SUMMARY