1RXS J232953.9+062814 slow fading continues Dear Colleagues, After the rebrightening observed on November 10-11, the star has shown a steady linear decline at a constant rate of 0.13 mag/d (at least up to Nov. 18). Such a linear post-superoutburst decline is rather frequently seen in WZ Sge-type dwarf novae or large-amplitude SU UMa-type dwarf novae, such as WX Cet (cf. Kato et al. 2001, PASJ 53, 893). Together with the presence of a post-superoutburst rebrightening, and double-humped light curve in quiescence, this star seems to bear characteristics similar to those of WZ Sge-type stars, as well as other peculiar properties already described. The short-term light curve is still dominated by double-wave humps, with occasional brightenings (time scale ~1-2 hr), during which humps tend to become rather unclear. The VSNET Collaboration team has received many new data, which will be reviewed later by Uemura-san. We have been also keenly analyzing all recent Kyoto observations, made on all nights. Please send any data and information to Uemura-san also (uemura@kusastro.kyoto-u.ac.jp). Regards, Taichi Kato VSNET Collaboration team