DM Lyr likely superoutburst: need for more observation Again a copy of the post to vsnet-alert. Since the object has not been seen in superoutburst in the past few years, the present (super?) outburst needs to be attended. However, the object would be the second priority until the nature of AW Sge becomes certain. The last likely superoutburst occurred in 1997 November-December. The 1996 July outburst led to the identification as a new member of SU UMa stars. More observations to precisely determine the superhumo period are encouraged. References: http://vsnet.kusastro.kyoto-u.ac.jp/vsnet/DNe/dmlyr.html http://vsnet.kusastro.kyoto-u.ac.jp/vsnet/DNe/dmlyrcom.html http://vsnet.kusastro.kyoto-u.ac.jp/vsnet/DNe/dmlyr9702.html YYYYMMDD(UT) mag observer 20000705.237 <154 (G. Hanson) 20000706.194 <154 (G. Hanson) 20000707.196 <160 (G. Hanson) 20000707.217 <130 (M. Simonsen) 20000709.424 <154 (G. Hanson) 20000710.283 <130 (M. Simonsen) 20000710.958 <154 (G. Poyner) 20000711.247 <130 (M. Simonsen) 20000711.976 143 (G. Poyner) 20000712.194 145: (M. Simonsen) Regards, Taichi Kato VSNET Collaboration team