Dear colleagues, New variable star discovery by the MISAO Project (MisV1081). MisV1081 R.A. 20h59m05s.15 Decl. +48o48'15".4 (2000.0) Mag. 10.3-12.2C Type SR? = IRAS 20574+4836 20h59m05s.3 +48o48'12" Ellipse:7x3" P.A.:168 Flux(12):3.026 Flux(25):1.340 Flux(60):<2.419 Flux(100):<36.46 Var:53% http://vsnet.aerith.net/misao/data/MisV/MisV1081.gif MisV1081 19990501.76068 10.29C Mis KAF-1600 - KenIchi_Kadota MisV1081 19990501.76113 10.31C Mis KAF-1600 - KenIchi_Kadota MisV1081 19990707.71403 11.23C Mis KAF-1600 - KenIchi_Kadota MisV1081 19990707.71453 11.23C Mis KAF-1600 - KenIchi_Kadota MisV1081 20001011.44535 12.19C Mis KAF-1600 - Nobuo_Ohkura MisV1081 20001011.44720 12.10C Mis KAF-1600 - Nobuo_Ohkura Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star MisV1081. 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/