Re: AQ Eri possible superoutburst > We are now observing AQ Eri at Kyoto. Its magunitude is ~13.6 mag. > It may be fainter than the magnitude for superoutburst. The current brightness seems to rather suggests a normal outburst. However, we would like to hear about any data on this outburst (the data should be directed to Ishioka-san (ishioka@kusastro.kyoto-u.ac.jp) or to vsnet-campaign-data@kusastro.kyoto-u.ac.jp). We would like observers to continue following the present outburst until it fades away. AQ Eri is similar to T Leo in its orbital period and outburst behavior. See also IBVS 4767 on our previous time-resolved photometry of an (apparently) normal outburst. Regards, VSNET Collaboration team