Dear colleagues, New variable star discovery by the MISAO Project (MisV1030). MisV1030 R.A. 20h31m21s.00 Decl. +33o36'46".8 (2000.0) Mag. 12.4C-13.8C Type ? = USNO-A2.0_1200.15249451 20 31 20.995 +33 36 46.75 14.5R 17.4B = IRAS 20293+3326 R.A.=20 31 21.64 Decl.=+33 36 49.4 (23 x 9", p.a.=68) flux(12)=0.97 flux(25)=0.51 flux(60)=<1.60 flux(100)=<79.05 93% variable http://vsnet.aerith.net/misao/data/MisV/MisV1030.gif MisV1030 19990605.74081 137C Mis image="KenIchi Kadota" MisV1030 19990605.74134 138C Mis image="KenIchi Kadota" MisV1030 20000803.53734 124C Mis image="Nobuo Ohkura" MisV1030 20000803.53919 125C Mis image="Nobuo Ohkura" Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star MisV1030. 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". 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/