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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
Return to the Powerful Daisaku Nogami
vsnet-adm@kusastro.kyoto-u.ac.jp
