V419 Lyr superhumps (Re: [vsnet-alert 3397] Nova Aql 99 and V 419 Lyr) The analysis of the combined set of Brno and Kyoto data has yielded the strong superhump signal around P=0.0968 d. This period is one of the longest among SU UMa-type dwarf novae, as Nogami et al. first suggested. More observations are strongly recommended. Regards, Taichi Kato and Rudolf Novak