The first metal enrichment in the universe was made by supernova ( SN ) explosions of population ( Pop ) III stars . The trace remains in abundance patterns of extremely metal-poor ( EMP ) stars . We investigate the properties of nucleosynthesis in Pop III SNe by means of comparing their yields with the abundance patterns of the EMP stars . We focus on ( 1 ) jet-induced SNe with various energy deposition rates [ \dot { E } _ { dep } = ( 0.3 - 1500 ) \times 10 ^ { 51 } ergs s ^ { -1 } ] , and ( 2 ) SNe of stars with various main-sequence masses ( M _ { ms } = 13 - 50 M _ { \odot } ) and explosion energies [ E = ( 1 - 40 ) \times 10 ^ { 51 } ergs ] . The varieties of Pop III SNe can explain varieties of the EMP stars : ( 1 ) higher [ C/Fe ] for lower [ Fe/H ] and ( 2 ) trends of abundance ratios [ X/Fe ] against [ Fe/H ] .