  We report the orbital distribution of the Trans-Neptunian objects (TNOs)
discovered during the High Ecliptic Latitude (HiLat) extension of the
Canada-France Ecliptic Plane Survey (CFEPS), conducted from June 2006 to July
2009. The HiLat component was designed to address one of the shortcomings of
ecliptic surveys (like CFEPS), their lack of sensitivity to high-inclination
objects. We searched 701~deg$^2$ of sky ranging from 12$^\circ$ to 85$^\circ$
ecliptic latitude and discovered \lKBO TNOs, with inclinations between
15$^\circ$ to 104$^\circ$. This survey places a very strong constraint on the
inclination distribution of the hot component of the classical Kuiper Belt,
ruling out any possibility of a large intrinsic fraction of highly inclined
orbits. Using the parameterization of \citet{2001AJ....121.2804B}, the HiLat
sample combined with CFEPS imposes a width $14^\circ \le \sigma \le
15.5^\circ$, with a best match for $\sigma = 14.5^\circ$. HiLat discovered the
first retrograde TNO, 2008~KV$_{42}$, with an almost polar orbit with
inclination 104$^\circ$, and (418993), a scattering object with perihelion in
the region of Saturn's influence, with $a \sim 400$~AU and $i = 68^\circ$.
