Dear colleagues, New variable star discovery by the MISAO Project (MisV1082). MisV1082 R.A. 21h01m24s.21 Decl. +49o22'59".3 (2000.0) Mag. 12.5-13.1C Type ? = IRAS 20597+4911 21h01m24s.4 +49o22'57" Ellipse:7x4" P.A.:170 Flux(12):1.315 Flux(25):0.8198 Flux(60):<2.999 Flux(100):<38.78 Var:12% http://vsnet.aerith.net/misao/data/MisV/MisV1082.gif MisV1082 19990501.76068 13.13C Mis KAF-1600 - KenIchi_Kadota MisV1082 19990501.76113 13.11C Mis KAF-1600 - KenIchi_Kadota MisV1082 20000918.47113 12.62C Mis KAF-1600 - Nobuo_Ohkura MisV1082 20000918.47298 12.52C Mis KAF-1600 - Nobuo_Ohkura MisV1082 20000918.47485 12.54C Mis KAF-1600 - Nobuo_Ohkura MisV1082 20001013.44513 12.84C Mis KAF-1600 - Nobuo_Ohkura MisV1082 20001013.44698 12.85C Mis KAF-1600 - Nobuo_Ohkura Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star MisV1082. It was picked up by Seiichi Yoshida from the candidates of new variable stars detected by the PIXY system 2 from images taken by Nobuo Ohkura comparing with images taken by KenIchi Kadota, and confirmed by KenIchi Kadota. The identification is researched by Taichi Kato (Kyoto University), John Greaves (the United Kingdom), and Seiichi Yoshida. The magnitude are measured automatically by the PIXY system 2. About the MISAO Project and the PIXY system 2: http://vsnet.aerith.net/misao/ -- Seiichi Yoshida comet@aerith.net http://vsnet.aerith.net/