I have updated my UBVRI bright-star field photometry file for WZ Sge: http://ftp.nofs.navy.mil/pub/outgoing/aah/sequence/wzsge.bright.dat This includes two photometric nights and two marginally photometric nights. The results are good; typical mean errors are under one percent. The V magnitudes differ from Krzeminski and Kraft; the colors are the same within error. Arlo Landolt has remeasured the three K&K stars and will give us the definitive answer in a couple of weeks. Arne