Discovery of strong CIV absorption in the highest redshift quasar

We report the near-IR detection of a prominent CIV absorption in the rest-f rame UV spectrum of the most distant known QSO, SDSS J104433.04-012502.2, a t z = 5.80. This QSO was recently observed with XMM-Newton and it was found to be notably X-ray weak. The equivalent width of the CIV absorption featu re (similar to 10 Angstrom) strongly supports the idea that the X-ray faint ness of this QSO is due to heavy absorption by gas with a column density N- H > 10(24) cm(-2). The shape of the CIV feature suggests that this is a Bro ad Absorption Line QSO. Although absorbed by a huge column of gas, the obse rved continuum in the 0.9-2.4 mum range (similar to 1300-3500 Angstrom rest frame) exactly matches the template of unabsorbed QSOs without invoking an y reddening (EB-V < 0.08 mag), indicating that dust in the absorbing gas is either absent or composed of large grains.