The minimum universal metal density between redshifts of 1.5 and 5.5

It appears that the Ly forest is becoming thick at a redshift of about 5.5, cutting off the higher redshift intergalactic medium from view in neutral hydrogen. However, the effects of star formation at higher redshift are sti ll readable in the intergalactic metal lines. In this Letter, I use observa tions of 32 quasars with emission redshifts in the range 2.31-5.86 to study the evolution of the intergalactic metal density from to z = 1.5 to z = 5. 5. The C IV column density distribution function is consistent with being i nvariant throughout this redshift range. From direct integration, I determi ne Omega (C IV) to be in the range and (2.5-7) x 10(-8) and Omega (Si IV) i n the range (0.9-3) x 10(-8) between z = 1.5 and z = 5. The metallicity at z = 5 exceeds 3.5 x 10(-4), which in turn implies that this fraction of the universal massive star formation took place beyond this redshift. This is sufficient to have ionized the intergalactic medium.