More precise data will be reported after the reduction. I thank T. Vanmunster and G. Poyner for notifying the current outburst. A preliminary analysis of the eclipse light curves has yielded following mid-eclipse times and eclipse depths. Due to the asymmetry of the eclipse light curves, these values would have a certain offset from the mid-eclipse times of the white dwarf. It is also interesting to note that the eclipse depth is indeed increasing.
Close monitoring is highly encouraged.
A preliminary analysis of the eclipse light curves has yielded following mid-eclipse times and eclipse depths. This table also contains the eclipse times on Feb. 27 for convenience. The eclipse times were not calculated for Feb. 28 and Mar. 1 observations due to the very poor photometric condition. Note that the asymmetry of the eclipse light curves may have resulted a certain offset from the mid-eclipse times of the white dwarf. We hope these eclipse times and period determination would be of any help in scheduling the further observations.