We present a homogeneous sample of 1361 L and T dwarfs brighter than J = 17.5 (of which 998 are new), from an effective area
of 3070 deg2, classified by the photo-type method to an accuracy of one spectral sub-type using izY JHKW1W2 photometry from
SDSS+UKIDSS+WISE. Other than a small bias in the early L types, the sample is shown to be effectively complete to the magnitude
limit, for all spectral types L0 to T8. The nature of the bias is an incompleteness estimated at 3% because peculiar blue L dwarfs of
type L4 and earlier are classified late M. There is a corresponding overcompleteness because peculiar red (likely young) late M dwarfs
are classified early L. Contamination of the sample is confirmed to be small: so far spectroscopy has been obtained for 19 sources in
the catalogue and all are confirmed to be ultracool dwarfs. We provide coordinates and izY JHKW1W2 photometry of all sources. We
identify an apparent discontinuity, ∆m ∼ 0.4 mag., in the Y − K colour between spectral types L7 and L8. We present near-infrared
spectra of nine sources identified by photo-type as peculiar, including a new low-gravity source ULAS J005505.68+013436.0, with
spectroscopic classification L2γ. We provide revised izY JHKW1W2 template colours for late M dwarfs, types M7 to M9.