Dear colleagues, New variable star discovery by the MISAO Project (MisV1025). MisV1025 R.A. 20h10m41s.34 Decl. +34o15'21".8 (2000.0) Mag. 11.4C-13.9C Type M? = USNO-A2.0_1200.14621290 20 10 41.340 +34 15 21.84 13.8R 18.9B = IRAS 20087+3406 R.A.=20 10 41.23 Decl.=+34 15 19.5 (23 x 5", p.a.=64) flux(12)=4.71 flux(25)=2.36 flux(60)=<5.50 flux(100)=<64.46 67% variable = 2MASS 201041.289 +341520.80 (2000.0) 6.057 0.000 0.000 http://vsnet.aerith.net/misao/data/MisV/MisV1025.gif MisV1025 19991121.41012 139C Mis image="KenIchi Kadota" MisV1025 20000803.52436 114C Mis image="Nobuo Ohkura" MisV1025 20000803.52620 114C Mis image="Nobuo Ohkura" Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star MisV1025. It was picked up by Yoshida from the candidates of new variable stars detected by the PIXY system from images taken by Ohkura comparing with images taken by Kadota. Kadota and Yoshida judged it as a real variable star. The magnitude are measured automatically by the PIXY system. Image observers' names are noted after "Mis". The identification with the 2MASS data is by Taichi Kato. Please see the URL below for the MISAO Project and the PIXY system. http://vsnet.aerith.net/misao/ -- Seiichi Yoshida comet@aerith.net http://vsnet.aerith.net/