  Mergers of spinning black holes can give recoil velocities from gravitational
radiation up to several thousand km/s. A recoiling supermassive black hole in
an AGN retains the inner part of its accretion disk. Marginally bound material
rejoining the disk around the moving black hole releases a large amount of
energy in shocks in a short time, leading to a flare in thermal soft X-rays
with a luminosity approaching the Eddington limit. Reprocessing of the X-rays
by the infalling material gives strong optical and ultraviolet emission lines
with a distinctive spectrum. Despite the short lifetime of the flare (~10^4
yr), as many as 100 flares may be in play at the present time in QSOs at
redshifts ~ 1 to 3. These flares provide a means to identify high velocity
recoils.
