We present the discovery of two z > 6 quasars, selected as i band dropouts in the VST ATLAS survey. Our first quasar has redshift, z = 6.31 pm 0.03, z band magnitude, z_AB = 19.63 pm 0.08 and rest frame 1450A absolute magnitude, M_1450 = -27.8 pm 0.2
, making it the joint second most luminous quasar known at z > 6. The second quasar has z = 6.02 pm 0.03, z_AB = 19.54 pm 0.08 and M_1450 = -27.0 pm 0.1. We also recover a z = 5.86 quasar discovered by Venemans et al. (2015, in prep.). To select our quasars we use a new 3D colour space, combining the ATLAS optical colours with mid-infra-red data from the Wide-field Infrared Survey Explorer (WISE). We use i_AB - z_AB colour to exclude main sequence stars, galaxies and lower redshift quasars, W1 - W2 to exclude L dwarfs and z_AB - W2 to exclude T dwarfs. A restrictive set of colour cuts returns only our three high redshift quasars and no contaminants, albeit with a sample completeness of ~50%. We discuss how our 3D colour space can be used to reject the majority of contaminants from samples of bright 5.7 < z < 6.3 quasars, replacing follow-up near-infra-red photometry, whilst retaining high completeness.
