I've placed on the anon ftp computer revised versions of both the Sumner sequence and the .dat field photometry file for this variable, based on two photometric nights. The errors are now closer to the truth. I repositioned the field on the second night to pick up a couple more comparison stars that are closer in color and magnitude to the Xray nova, and inserted them into Bruce's sequence. Note that the field photometry file includes UBVRI results, not just BV as listed on the sequence. Arne