  Although many new brown dwarf (BD) neighbours have recently been discovered
thanks to new sky surveys in the mid- and near-infrared (MIR, NIR), their
numbers are still more than five times lower than those of stars in the same
volume. Our aim is to detect and classify new BDs to eventually complete their
census in the immediate Solar neighbourhood. We combined multi-epoch data from
sky surveys at different wavelengths to detect BD neighbours of the Sun by
their high proper motion (HPM). We concentrated at relatively bright MIR
(w2<13.5) BD candidates from WISE expected to be so close to the Sun that they
may also be seen in older NIR (2MASS, DENIS) or even red optical (SDSS i- and
z-band, SSS I-band) surveys. With low-resolution NIR spectroscopy we classified
the new BDs and estimated their distances and velocities. We have discovered
the HPM (pm~470mas/yr) T7.5 dwarf, WISE J0521+1025, which is at d=5.0+-1.3pc
from the Sun the nearest known T dwarf in the northern sky, and two early-T
dwarfs, WISE J0457-0207 (T2) and WISE J2030+0749 (T1.5), with proper motions of
~120 and ~670mas/yr and distances of 12.5+-3.1pc and 10.5+-2.6pc, respectively.
The last one was independently discovered and also classified as a T1.5 dwarf
by Mace and coworkers. All three show thin disk kinematics. They may have been
overlooked in the past owing to overlapping images and because of problems with
matching objects between different surveys and measuring their proper motions.
