A luminous quasar at a redshift of z = 7.085
  The intergalactic medium was not completely reionized until approximately a
billion years after the Big Bang, as revealed by observations of quasars with
redshifts of less than 6.5. It has been difficult to probe to higher redshifts,
however, because quasars have historically been identified in optical surveys,
which are insensitive to sources at redshifts exceeding 6.5. Here we report
observations of a quasar (ULAS J112001.48+064124.3) at a redshift of 7.085,
which is 0.77 billion years after the Big Bang. ULAS J1120+0461 had a
luminosity of 6.3x10^13 L_Sun and hosted a black hole with a mass of 2x10^9
M_Sun (where L_Sun and M_Sun are the luminosity and mass of the Sun). The
measured radius of the ionized near zone around ULAS J1120+0641 is 1.9
megaparsecs, a factor of three smaller than typical for quasars at redshifts
between 6.0 and 6.4. The near zone transmission profile is consistent with a Ly
alpha damping wing, suggesting that the neutral fraction of the intergalactic
medium in front of ULAS J1120+0641 exceeded 0.1.
