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[vsnet-alert 4248] SW UMa




 We have observed 7045 frames of SW UMa from Feb. 12 to 18 and 
Dr. Martin also observed 535 frames on Feb. 17 and 18.  
We did not detect the super-QPO during the very early stage of 
superoutburst.  From Feb. 15, the object is gradually faded 
with the rate of  0.13 mag/d.  The amplitude of superhump is 
constant after fully evolved to about 2.0 mag.

 Tonight we are now observing SW UMa.  The object is sometimes 
visible on display through thin cloud, but the condition is 
not good.  The other site observations are encouraged. 

Regards,
Makoto Uemura and Taichi Kato

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