The discovery of the first luminous z ∼ 6 quasar in the UKIDSS Large Area Survey

We present the initial results from our search for high-redshift, z greater than or similar to 6, quasars using near-infrared (near-IR) data from the UKIRT Infrared Deep Sky Survey Large Area Survey. Our analysis of 106 deg(2) of sky from Data Release 1 has resulted in the discovery of ULAS J020332.38+001229.2, a luminous (J(AB) = 20.0, J(Vega) = 19.1, M-1450 = -26.2) quasar at z = 5.86. Following candidate selection from the combined IR and optical catalogue data and stacking of multiple epoch Sloan Digital Sky Survey (SDSS) data, we have obtained optical spectroscopy for the only two z greater than or similar to 6 quasar candidates. The Very Large Telescope FORS2 spectrum of ULAS J020332.38+001229.2 shows broad Ly alpha + N V 1240 emission at similar to 8350 angstrom and an abrupt continuum break due to absorption by the Lya forest. The quasar is not present in the SDSS DR5 catalogue and the continuum spectral index of alpha = -1.4 (F-nu proportional to nu(alpha)) is redder than a composite of SDSS quasars at similar redshifts (alpha = -0.5). The discovery of one z similar to 6 quasar in similar to 100 deg(2) in a complete sample within our selection criteria down to a median depth of Y-AB = 20.4 (7 sigma) is consistent with existing SDSS results. We describe our survey methodology, including the use of optical data from the SDSS and the highly effective procedures developed to isolate the very small surface density of high-probability quasar candidates.