Dear colleagues, New variable star discovery by the MISAO Project (MisV1139). MisV1139 R.A. 21h46m27s.85 Decl. +49o42'05".5 (2000.0) Mag. 12.2-13.2C Type ? = USNO-A2.0 1350.14919665 21h46m27s.805 +49o42'06".35 Mag(R):14.7 Mag(B):17.8 = IRAS 21446+4928 21h46m26s.6 +49o41'60" Ellipse:38x10" P.A.:52 Flux(12):0.5403 Flux(25):0.2685 Flux(60):<0.4000 Flux(100):<10.79 Var:50% http://vsnet.aerith.net/misao/data/MisV/MisV1139.gif MisV1139 19990724.63284 13.21C Mis KAF-1600 - KenIchi_Kadota MisV1139 19990724.63327 13.13C Mis KAF-1600 - KenIchi_Kadota MisV1139 20000805.57009 12.48C Mis KAF-1600 - Nobuo_Ohkura MisV1139 20000805.57194 12.31C Mis KAF-1600 - Nobuo_Ohkura MisV1139 20000805.57379 12.29C Mis KAF-1600 - Nobuo_Ohkura MisV1139 20000810.55186 12.17C Mis KAF-1600 - Nobuo_Ohkura MisV1139 20000810.55371 12.23C Mis KAF-1600 - Nobuo_Ohkura MisV1139 20000902.52742 12.31C Mis KAF-1600 - Nobuo_Ohkura MisV1139 20001013.47109 12.30C Mis KAF-1600 - Nobuo_Ohkura MisV1139 20001013.47296 12.38C Mis KAF-1600 - Nobuo_Ohkura MisV1139 20001013.47482 12.40C Mis KAF-1600 - Nobuo_Ohkura Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star MisV1139. 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/