The black hole itself does not emit the radiation, but rather the space just around it. Because of quantum effects, small particles and anti-particles will spontaneously create everywhere (and later annihilate themselves in a collision). If this happens just outside the event horizon, one particle will inevitably fall into it, never to be seen again. The other particle is now 'free' and this is the radiation Hawking predicted.
Can we detect a black hole's radiation?
Well, this radiation is way too small to be detected by itself, even if the black hole would be at our doorstep. However, the radiation makes the black hole less massive and smaller and finally it will vanish, producing a gamma ray flash which we hope is detectable, even from a very large distance.
As @JamesK notes in the comments, this evaporation will take extremely long for the 'common' black holes caused by supernovae and those found in galaxy centers, but smaller primordial black holes, formed in the very beginning of the universe, could be evaporating now and that's why we have a telescope looking for those gamma ray flashes.