Dear colleagues, New variable star discovery by the MISAO Project (MisV1042). MisV1042 R.A. 19h59m44s.68 Decl. +42o00'13".2 (2000.0) Mag. 8.8-10.0C Type SR: = IRAS 19580+4151 19h59m44s.4 +42o00'11" Ellipse:19x4" P.A.:63 Flux(12):29.35 Flux(25):12.25 Flux(60):1.671 Flux(100):<75.64 Var:99% = 2MASS 195944.658 +420013.14 (2000.0) 6.607 5.350 0.000 http://vsnet.aerith.net/misao/data/MisV/MisV1042.gif MisV1042 19990430.68636 9.26C Mis KAF-1600 - KenIchi_Kadota MisV1042 19990430.68679 9.30C Mis KAF-1600 - KenIchi_Kadota MisV1042 19990724.58430 10.00C Mis KAF-1600 - KenIchi_Kadota MisV1042 19990724.58475 9.98C Mis KAF-1600 - KenIchi_Kadota MisV1042 20000907.46204 8.77C Mis KAF-1600 - Nobuo_Ohkura MisV1042 20000907.46389 8.83C Mis KAF-1600 - Nobuo_Ohkura Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star MisV1042. 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/