1. Introduction

2. Target Selection for FMOS Observation  
2.1. Input Photometric Galaxy Catalogues for Selection  
2.2. Color-based Selection  
2.3. Selection by Photometric Redshifts and Hα Flux Estimation  

3. FMOS Observation  
3.1. Observation and Data Reduction  
3.2. Emission Line Detection  

4. Results and Discussion  
4.1. Statistics of Line Detection  
4.2. Spectroscopic versus Photometric Estimates of Redshift and Hα Flux  
4.3. Comparison with the HiZELS Data  

5. Conclusion