Dear Makoto, it is so nice to hear these news! later today I will be joining observig, in order to have a longer coverage. Any informatiuon about the recommended reference stars are welcomed! Keep up the good work, Gianluca Scrive Makoto Uemura <uemura@kusastro.kyoto-u.ac.jp>: > > WZ Sge: rapidly brightening! > > Our preliminary photometry of WZ Sge shows a rapidly brightening > of the object. We started time-series observation at 14:30 (UT) and > the object was about 9.5mag at that time, and then, now (17:00 UT) we > estimate the object is about 9.1mag, which indicates the rising rate > is about 3.8 mag/day. > > As in the recent case of RZ Leo and AL Com, WZ Sge stars show > "early superhump" during the very early phase of their outbursts. > Tonight observations are important to study the birth of early > superhumps. > As well as follow-up photometric observations, tonight spectroscopy is > > strongly urged. > > As reported by Dr. Kuulkers, the object may show short-period > oscillations during the rising phase, so observers should take CCD > images with an exposure time as short as possible. > The Kyoto team is now observing with an exposure time of 10s > (25-cm SC + ST-7E). > > Regards, > Makoto Uemura > >