Dear colleagues, New variable star discovery by the MISAO Project (MisV1067). MisV1067 R.A. 22h38m07s.93 Decl. +54o51'53".8 (2000.0) Mag. 11.4-12.5C Type ? = USNO-A2.0 1425.13785050 22h38m08s.106 +54o51'54".42 Mag(R):12.1 Mag(B):14.5 = IRAS 22361+5436 22h38m07s.9 +54o51'53" Ellipse:9x9" P.A.:29 Flux(12):0.8317 Flux(25):0.2576 Flux(60):<0.4000 Flux(100):<13.14 Var:44% http://vsnet.aerith.net/misao/data/MisV/MisV1067.gif MisV1067 19990821.74924 12.41C Mis KAF-1600 - KenIchi_Kadota MisV1067 19990821.74967 12.49C Mis KAF-1600 - KenIchi_Kadota MisV1067 20000829.53505 11.44C Mis KAF-1600 - Nobuo_Ohkura MisV1067 20000829.53691 11.45C Mis KAF-1600 - Nobuo_Ohkura MisV1067 20000829.53875 11.42C Mis KAF-1600 - Nobuo_Ohkura Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star MisV1067. 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/