WZ Sge: new data and nightly averaged magnitudes Dear Colleagues, We have received new data from the following observers: D. Starkey, B. Martin (two nights), J. Pietz (one full night and one partially analyzed set), RIT observatory (M. Richmond, S. Davis, D. Crabtree, K. Beaulieu). Thank you for all observers! We are currently analyzing the Kyoto Aug. 15 data (full night coverage). Nightly averaged magnitudes, as usual, clearly show that WZ Sge has almost completely stopped fading! The brightest epoch seems to correspond to the stage when superhumps have an "M"-shaped profile. More analysis and Web information will follow later. mid-UT V-C err N -------------------------------- 20010723.774 0.087 0.012 1665 20010724.704 -0.469 0.002 3906 20010725.610 -0.216 0.002 5947 20010726.686 -0.063 0.002 1848 20010727.588 0.099 0.001 8386 20010728.686 0.318 0.002 3985 20010729.515 0.410 0.001 5752 20010730.667 0.571 0.001 5316 20010731.636 0.687 0.001 6042 20010801.630 0.777 0.001 9440 20010802.470 0.900 0.002 2379 20010803.614 0.984 0.001 6197 20010804.634 1.095 0.001 5103 20010805.529 1.144 0.001 6850 20010806.464 1.177 0.002 2800 20010807.493 1.255 0.002 1976 20010808.513 1.306 0.001 3293 20010809.632 1.352 0.002 2079 20010810.567 1.449 0.001 3265 20010811.516 1.565 0.001 8617 20010812.518 1.698 0.001 3529 20010813.563 1.819 0.001 6400 20010814.631 1.884 0.001 5038 20010815.292 1.899 0.001 3612 Regards, Taichi Kato VSNET Collaboration team