V592 Her linearly fading Nightly averages of Garradd's CCD time series indicate V592 Her is linearly fading, as is usual for a superoutburst. The average rate 0.21 mag/day is significantly larger than usual SU UMa type dwarf novae. mid-UT mean S.D. N observer ---------------------------------------- 980830.421 14.138 0.116 130 GAR 980901.392 14.581 0.065 10 GAR 980902.418 14.757 0.107 194 GAR (The zero point of mean magnitudes are rather arbitrary; these calibrations seem to give slightly fainter magnitudes than visual estimates). Masi's CCD observation on Aug. 31 seems to safely preclude large-amplitude superhumps. Regards, Taichi Kato