Dear colleagues, New variable star discovery by the MISAO Project (MisV1052). MisV1052 R.A. 20h14m42s.85 Decl. +43o17'32".6 (2000.0) Mag. 12.1-12.7C Type SR? = USNO-A2.0 1275.13701869 20h14m42s.779 +43o17'32".46 Mag(R):15.5 Mag(B):19.8 = IRAS 20130+4308 20h14m42s.5 +43o17'31" Ellipse:20x4" P.A.:63 Flux(12):1.555 Flux(25):1.010 Flux(60):<22.64 Flux(100):<185.4 Var:1% = 2MASS 201442.738 +431731.74 (2000.0) 7.065 5.694 5.061 http://vsnet.aerith.net/misao/data/MisV/MisV1052.gif MisV1052 19990803.69073 12.65C Mis KAF-1600 - KenIchi_Kadota MisV1052 19990803.69117 12.56C Mis KAF-1600 - KenIchi_Kadota MisV1052 19991121.42256 12.27C Mis KAF-1600 - KenIchi_Kadota MisV1052 19991121.42299 12.33C Mis KAF-1600 - KenIchi_Kadota MisV1052 20000904.47315 12.06C Mis KAF-1600 - Nobuo_Ohkura Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star MisV1052. It was picked up by Seiichih 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/