I've placed on http://ftp.nofs.navy.mil/pub/outgoing/aah/sequence/sn2000ce.dat the BVRI field photometry for this supernova based on a single photometric night. Potential zeropoint offsets of 0.02mag are possible, however the current file is more than adequate for visual observers. All stars brighter than V=12.5 are saturated and should be used with care. The magnitudes on the Puckett finding chart the AAVSO has on their website are close to true V, with a few stars deviating by up to 0.2mag. arne