There are only THREE helium dwarf novae. CR Boo, V803 Cen and CP Eri. Schwarz's discovery of "SN1998di" adds a great new specimen to this unique subgroup of dwarf novae. Observations are highly encouarged, are we are happy to receive observations (e.g. to vsnet-obs or to myself, either from the CV or SN communities) and feed back new fidings. All of the known three helium dwarf novae show very short-term variation (orbital period tens of miniutes, outburst-like oscillations every sub-day to days, and superoutburst quasi-periodically repeating with a typical time-scale of tens of days. Continued observations by the same instrument, with which one may gain aditional possibility of catching a supernova than by watching field CVs, is highly encouraged. The USNO A1.0-based (V-equivalent) VSNET chart [vsnet-chart 66] is available at: http://vsnet.kusastro.kyoto-u.ac.jp/vsnet/Mail/vsnet-chart/msg00066.html (Original image by the discoverer: http://vsnet2.netcom.com/~pfactors/tenagra.html) Regards, Taichi Kato