I've posted on http://ftp.nofs.navy.mil/pub/outgoing/aah/sequence/v1494aql.dat the UBVRI field photometry file for this nova based on two photometric nights. The nova is still too bright for this file to be of value for visual observers, but it should be useful for CCD observers. Note that this is a reddened field; it is difficult to find stars of comparable color to the nova. The crowding is such that you should not trust the photometry for any given object until you have checked a CCD/DSS frame to be sure no neighbors are contaminating the measures. Arne