1. INTRODUCTION
2. THE SUBARU DEEP FIELD
2.1. Selection of Emission-line Galaxies
2.2. Optical Spectroscopy
2.3. Accurate Flux Calibration of MMT and Keck Spectra
3. THE [O III] λ4363-NON-DETECTED SAMPLE
4. Te AND METALLICITY DETERMINATIONS
4.1. Dust-corrected SFRs
4.2. SEDs and Stellar Masses
4.3. ISM Gas Densities
5. CONCLUSIONS