Dear colleagues, New variable star discovery by the MISAO Project (MisV1073). MisV1073 R.A. 20h01m44s.24 Decl. +46o58'20".8 (2000.0) Mag. 11.3-11.8C Type SR: = USNO-A2.0 1350.11491324 20h01m44s.228 +46o58'21".44 Mag(R):13.6 Mag(B):15.8 = IRAS 20001+4649 20h01m42s.6 +46o58'21" Ellipse:38x9" P.A.:65 Flux(12):0.3021 Flux(25):<0.2500 Flux(60):<0.5274 Flux(100):<42.48 = 2MASS 200144.208 +465820.68 (2000.0) 7.980 6.940 6.539 http://vsnet.aerith.net/misao/data/MisV/MisV1073.gif MisV1073 19990430.68129 11.62C Mis KAF-1600 - KenIchi_Kadota MisV1073 19990430.68171 11.60C Mis KAF-1600 - KenIchi_Kadota MisV1073 19990724.60014 11.34C Mis KAF-1600 - KenIchi_Kadota MisV1073 19990724.60056 11.30C Mis KAF-1600 - KenIchi_Kadota MisV1073 20000917.44029 11.80C Mis KAF-1600 - Nobuo_Ohkura MisV1073 20000917.44215 11.82C Mis KAF-1600 - Nobuo_Ohkura MisV1073 20000917.44400 11.81C Mis KAF-1600 - Nobuo_Ohkura MisV1073 20001009.41291 11.67C Mis KAF-1600 - Nobuo_Ohkura MisV1073 20001009.41475 11.58C Mis KAF-1600 - Nobuo_Ohkura MisV1073 20001009.41661 11.54C Mis KAF-1600 - Nobuo_Ohkura Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star MisV1073. 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/