I've not got figures to hand, but it's incredibly slow. They are effectively perfect black body radiators, with their apparent temperature linked to their mass. The bigger they are, the colder they are.
Some back of the envelope calculations.
Right now, they are considerably colder than the cosmic background radiation, and so losses to hawking radiation are overwhelmed by even this. I just did a quick calculation on the milk way supermassive black hole, and it's about 1.5x10^-16 °C. That would work out as around 3x10^-91W/m^2 or around 1x10^-71W. It's about 1x10^13 Joules per gram of matter. So you're looking at 10^84 seconds. The universe is about 4.4x10^16 seconds old, so around 10^68 times the current age of the universe.
To emit 1g will take around 100000000000000000000000000000000000000000000000000000000000000000000 x the age of the current universe. This ignores infalling energy.