Iron Emission in z 6 QSO s

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Abstract
We have obtained low-resolution near-infrared spectra of three QSOs at 5.7 < z < 6.3 using the Near-Infrared Camera and Multi-Object Spectrometer on the Hubble Space Telescope. The spectra cover the rest-frame ultraviolet emission of the objects between λrest ≈ 1600 and 2800 Å. The Fe II emission-line complex at 2500 Å is clearly detected in two of the objects and possibly detected in the third. The strength of this complex and the ratio of its integrated flux to that of Mg II λ2800 are comparable to values measured for QSOs at lower redshifts and are consistent with Fe/Mg abundance ratios near or above the solar value. There thus appears to be no evolution of QSO metallicity to z ≈ 6. Our results suggest that massive, chemically enriched galaxies formed within 1 Gyr of the big bang. If this chemical enrichment was produced by Type Ia supernovae, then the progenitor stars formed at z ≈ 20 ± 10, in agreement with recent estimates based on the cosmic microwave background. These results also support models of an evolutionary link between star formation, the growth of supermassive black holes, and nuclear activity.
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