V1028 Cyg We obtained four hours' CCD photometry between July 30.63 and 30.81. The light curve clearly indicates that "true" superhumps have grown. The amplitude of superhumps has grown to 0.07 mag, with a familiar single- peaked hump structure. A prelimiary period analysis yields the best estimate of the superhump period as 0.065 +/- 0.001 day (slightly affected by short duration of the run). It is curious that the period reported for July 29 observations was significantly longer. We have re-analyzed the last night' data, by selecting high S/N data, and obtained a period of 0.070 +/- 0.001 day, which is still longer than the current value. We can not say at this time the cause of this discrepancy in periods. (An analysis of merged data set of these two nights shows marked periodicities at 0.0661 and 0.0704 day.) Of course this may be caused by limited duration of observations, intrinsic irregularity, unstable periodicity at the growing stage of super- humps, co-existence of double periods, etc. We should wait further obser- vations to check these possibilities. Anyway, we can now firmly say that V1028 Cyg is a genuine member of SU UMa-type dwarf novae. We will be observing for coming nights to follow the development of superhumps. Regards, Taichi Kato & Ouda Team