Dear colleagues, New variable star discovery by the MISAO Project (MisV1050). MisV1050 R.A. 20h08m58s.87 Decl. +41o47'08".6 (2000.0) Mag. 12.0-13.3C Type SR: = USNO-A2.0 1275.13500676 20h08m58s.997 +41o47'08".68 Mag(R):15.8 Mag(B):19.5 = IRAS 20072+4138 20h08m59s.3 +41o47'05" Ellipse:23x3" P.A.:64 Flux(12):0.5830 Flux(25):0.1936 Flux(60):1.782 Flux(100):<48.01 Var:0% = 2MASS 200858.992 +414708.65 (2000.0) 7.988 6.844 6.306 http://vsnet.aerith.net/misao/data/MisV/MisV1050.gif MisV1050 19990803.68972 12.03C Mis KAF-1600 - KenIchi_Kadota MisV1050 19990803.69016 11.97C Mis KAF-1600 - KenIchi_Kadota MisV1050 19991121.42156 12.78C Mis KAF-1600 - KenIchi_Kadota MisV1050 19991121.42201 12.66C Mis KAF-1600 - KenIchi_Kadota MisV1050 20000907.46946 13.26C Mis KAF-1600 - Nobuo_Ohkura Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star MisV1050. 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/