Dear colleagues, New variable star discovery by the MISAO Project (MisV1137). MisV1137 R.A. 21h32m29s.76 Decl. +49o43'23".3 (2000.0) Mag. 13.1-14.4C Type SR: = IRAS 21307+4930 21h32m30s.0 +49o43'26" Ellipse:10x9" P.A.:40 Flux(12):0.6108 Flux(25):0.2382 Flux(60):<0.5014 Flux(100):<13.69 Var:12% http://vsnet.aerith.net/misao/data/MisV/MisV1137.gif MisV1137 19990709.67729 14.44C Mis KAF-1600 - KenIchi_Kadota MisV1137 19990709.67786 14.41C Mis KAF-1600 - KenIchi_Kadota MisV1137 20000805.56452 14.24C Mis KAF-1600 - Nobuo_Ohkura MisV1137 20000805.56637 14.44C Mis KAF-1600 - Nobuo_Ohkura MisV1137 20000810.54259 13.90C Mis KAF-1600 - Nobuo_Ohkura MisV1137 20000810.54444 14.07C Mis KAF-1600 - Nobuo_Ohkura MisV1137 20000902.51629 13.49C Mis KAF-1600 - Nobuo_Ohkura MisV1137 20000902.51814 13.44C Mis KAF-1600 - Nobuo_Ohkura MisV1137 20000913.50979 13.41C Mis KAF-1600 - Nobuo_Ohkura MisV1137 20000913.51164 13.42C Mis KAF-1600 - Nobuo_Ohkura MisV1137 20001013.46182 13.18C Mis KAF-1600 - Nobuo_Ohkura MisV1137 20001013.46367 13.12C Mis KAF-1600 - Nobuo_Ohkura MisV1137 20001013.46553 13.14C Mis KAF-1600 - Nobuo_Ohkura Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star MisV1137. 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/