LX Ser activity? Recent observations suggests that the eclipsing novalike object LX Ser tends to vary in greater amplitudes than in recent years. This may be a signature of weak dwarf nova-type activity. The past long-lasting "NL"-state may have been extended standstills. If the current activity leads to dwarf nova outbursts, this eclipsing system may provide a unique opportunity to investigate the disk structure of Z Cam-type dwarf nova. Careful and continued observations are strongly encourged. CCD observers are also suggested to monitor this object to see whether reported variation actually reflects dwarf nova-type variation. If the variability is confirmed, eclipse observations are strongly requested. Please forward your findings to vsnet-campaign. YYYYMMDD(UT) mag observer 20000423.040 152 (G. Poyner) 20000424.231 149 (G. Hanson) 20000425.226 149 (G. Hanson) 20000425.238 <140 (M. Simonsen) 20000428.240 147 (G. Hanson) 20000430.028 151 (G. Poyner) 20000430.219 155: (G. Hanson) 20000430.256 <143 (M. Simonsen) 20000430.424 148 (G. Hanson) 20000501.007 151 (G. Poyner) 20000502.012 150 (G. Poyner) 20000502.172 142 (M. Simonsen) 20000502.199 148 (G. Hanson) 20000503.206 143 (G. Hanson) 20000503.233 <140 (M. Simonsen) 20000503.416 148 (G. Hanson) 20000504.224 147 (G. Hanson) 20000504.419 148 (G. Hanson) 20000505.262 147 (G. Hanson) 20000506.191 148 (G. Hanson) 20000507.269 146 (G. Hanson) 20000507.972 153 (G. Poyner) 20000509.417 <160 (G. Hanson) 20000509.430 149 (G. Hanson) 20000510.219 148 (G. Hanson) 20000511.405 147 (G. Hanson) 20000513.405 149 (G. Hanson) 20000514.976 151: (G. Poyner) 20000519.956 151 (G. Poyner) 20000521.967 152 (G. Poyner) 20000522.174 150 (G. Hanson) 20000523.255 149 (G. Hanson) 20000524.001 155 (G. Poyner) 20000524.244 149 (G. Hanson) 20000525.217 151 (G. Hanson) 20000526.233 145 (G. Hanson) 20000526.255 142 (M. Simonsen) 20000526.897 147 (M. Reszelski) 20000527.242 149 (G. Hanson) Regards, Taichi Kato VSNET Collaboration team