V419 Lyr superoutburst According to Pietz's observations (vsnet-obs 15708, http://vsnet.kusastro.kyoto-u.ac.jp/vsnet/Mail/obs15000/msg00708.html), the long-period SU UMa star V419 Lyr is definitely in superoutbrust. The object being in declining stage, any intended time-resolved photometry should be an urgent task. The likely supercycle length inferred from previous observations is around 300-400 days. YYMMDD(UT) mag observer 980901.940 <154 (T. Kinnunen) 980902.910 <154 (T. Kinnunen) 980903.869 <154 (T. Kinnunen) 980905.950 <148 (T. Kinnunen) 980907.930 <143 (T. Kinnunen) 980913.849 <154 (T. Kinnunen) 980920.880 148 (J. Pietz) 980921.869 149: (J. Pietz) 980921.890 <148 (T. Kinnunen) 980922.830 153 (T. Kinnunen) 980922.869 <146 (J. Pietz) 980923.819 153 (T. Kinnunen) 980924.810 158 (T. Kinnunen) 980925.819 160 (T. Kinnunen) Regards, Taichi Kato