Abstract
We present sensitive near-infrared (NIR) VLT ISAAC spectroscopic observations of the z = 6.08 quasar SDSS J030331.40-001912.9. This quasi-stellar object (QSO) is more than a magnitude fainter than other QSOs at z {approx} 6 for which NIR spectroscopy has been obtained to date and is therefore presumably more representative of the QSO population at the end of cosmic reionization. Combining rest-frame UV continuum luminosity with the width measurements of the Mg II and C IV lines, we derive a black hole mass of 2{sup +1.0} {sub -0.5} x 10{sup 8} M {sub sun}, the lowest mass observed for z {approx} 6 QSOs to date, and derive an Eddington ratio of 1.6{sup +0.4} {sub -0.6}, among the highest value derived for QSOs at any redshift. The Spitzer 24 {mu}m nondetection of this QSO does not leave space for a significant hot dust component in its optical/NIR spectral energy distribution, in common with one other faint QSO at z = 6, but in contrast to more than 20 more z = 6 QSOs and all known lower redshift QSOs with sufficiently deep multiwavelength photometry. We conclude that we have found evidence for differences in the intrinsic properties of at least one z more » {approx} 6 QSO as compared to the lower redshift population. « less
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