Dear colleagues, New variable star discovery by the MISAO Project (MisV0826). MisV0826 R.A. 16h58m11s.32 Decl. -23o31'07".6 (2000.0) Mag. 11.8C-13.4C Type ? = USNO-A2.0_0600.22644804 16 58 11.321 -23 31 07.57 15.6R 16.2B = IRAS 16551-2326 R.A.=16 58 12.85 Decl.=-23 31 11.3 (51 x 8", p.a.=97) flux(12)=0.47 flux(25)=<0.37 flux(60)=<0.40 flux(100)=<13.27 http://vsnet.aerith.net/misao/data/MisV/MisV0826.gif MisV0826 19990801.50869 118C Mis MisV0826 19990801.50990 118C Mis MisV0826 20000224.80469 134C Mis MisV0826 20000224.80523 133C Mis It was detected by the PIXY system as one of the candidates of new variable stars from images taken by KenIchi Kadota, Ageo City, Saitama, Japan, then confirmed by Seiichi Yoshida. The magnitude are measured automatically by the PIXY system. Image observers' names are noted after "Mis", except for ones taken by KenIchi Kadota. Please see the URL below for the MISAO Project and the PIXY system. http://vsnet.aerith.net/misao/ -- Seiichi Yoshida comet@aerith.net http://vsnet.aerith.net/