Dear Colleagues, last night I observed this star with the 0.8-m, f/8 reflector of Campo Catino Astronomical Observatory, with a R Bessel filter. I observed with Franco Mallia. Unfortunately, the clouds forced us to end observations after only one hour. A quick look to the resulting photometry show a probable, broad late-superhump. I will be sending our data to Kyoto, once it will be properly reduced. We provide astrometry for this target: R.A.:20 23 38.20; Decl.: +64 36 26.8 (J2000.0) 100 reference stars from USNO A2.0; mean residuals = 0.2" On Oct. 18.770, 2002, the star was at mag. 16.5Rc (we used the R magnitudes from USNO A2.0 for the reference stars). Regards, Gianluca Masi