HT Cam: continous light curve on Dec. 30 Thanks to the full data set by Gary Billings, we now have a complete coverage on Dec. 30! There is an indication of two different stages of decline. The first part resembles that of a plateau portion of a dwarf nova outburst, with a slower decline, low amplitude of orbital (or superhump) signals, and low amplitude of the 8 min signal. This part apparently lasted since the initial detection by Itoh. The latter part, which we have been mostly referring to, shows much more rapid decline, large amplitudes of orbital (or superhump) and 8-min signals. We have further received full-night data from Torii-san (RIKEN) on Dec. 31, which will be analyzed soon. Regards, Taichi Kato VSNET Collaboration team