A reanalysis of data taken on the Cygnus region in 1989-90 using the Whipple Observatory atmospheric Cherenkov imaging telescope confirms the existence of the TeV J2032+4130 source reported by the Crimean Astrophysical Observatory and published by the HEGRA Collaboration .
The significance at the a priori HEGRA position is 3.3 \sigma .
The peak signal was found at RA = 20h32m , Dec = +41 ^ { \circ } 33 ’ .
This is 0.6 ^ { \circ } north of Cygnus X-3 which was the original target of the observations .
The flux level ( 12 % of the level of the Crab Nebula ) is intermediate between the two later observations and suggests that the TeV source is variable .