Dear colleagues, New variable star discovery by the MISAO Project (MisV1066). MisV1066 R.A. 22h29m25s.48 Decl. +55o14'04".9 (2000.0) Mag. 11.3-11.8C Type ? = USNO-A2.0 1425.13511025 22h29m25s.471 +55o14'03".95 Mag(R):14.1 Mag(B):17.5 = IRAS 22274+5458 22h29m25s.7 +55o14'05" Ellipse:14x8" P.A.:22 Flux(12):0.5899 Flux(25):0.3095 Flux(60):<1.731 Flux(100):<17.09 Var:0% http://vsnet.aerith.net/misao/data/MisV/MisV1066.gif MisV1066 19990709.70923 11.25C Mis KAF-1600 - KenIchi_Kadota MisV1066 19990709.70966 11.26C Mis KAF-1600 - KenIchi_Kadota MisV1066 20000829.52950 11.76C Mis KAF-1600 - Nobuo_Ohkura MisV1066 20000829.53135 11.71C Mis KAF-1600 - Nobuo_Ohkura Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star MisV1066. 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/