1. INTRODUCTION  
2. OBSERVATIONS AND DATA REDUCTION  
2.1. The target galaxies  
2.2. Data reduction and calibration  
3. METHOD  
3.1. Grid-shaped aperture photometry  
3.2. SED modeling  
4. RESULTS  
4.1. Photometric properties  
5. DISCUSSION  
5.1. Internal attenuation  
5.2. Metallicity  
5.3. LyC escape  
5.4. Star formation history  
5.5. Uncertainty of the Hα flux calibration  
6. SUMMARY