A method has been developed to search for pulsed and/or unpulsed ultra
-high-energy (UHE) emission point sources over a range of time scales.
This method has been applied to data accumulated with the CYGNUS exte
nsive air-shower array to search for episodic emission from Cyg X-3, H
er X-1, the Crab Nebula, and a collection of 48 secondary source candi
dates. An examination of timescales ranging from minutes to years has
yielded results consistent with background fluctuations.