Dear colleagues, New variable star discovery by the MISAO Project (MisV0925). MisV0925 R.A. 19h31m06s.80 Decl. +10o28'08".5 (2000.0) Mag. 11.2C-12.7C Type ? = USNO-A2.0_0975.15097044 19 31 06.795 +10 28 08.52 15.3R 18.1B = IRAS 19287+1021 R.A.=19 31 06.38 Decl.=+10 28 05.2 (42 x 8", p.a.=78) flux(12)=0.86 flux(25)=0.28 flux(60)=<0.40 flux(100)=<22.50 0% variable http://vsnet.aerith.net/misao/data/MisV/MisV0925.gif MisV0925 19990605.67561 114C Mis image="KenIchi Kadota" MisV0925 19990605.67606 113C Mis image="KenIchi Kadota" MisV0925 19990605.67667 116C Mis image="KenIchi Kadota" MisV0925 19990605.67709 116C Mis image="KenIchi Kadota" MisV0925 19990923.55779 127C Mis image="KenIchi Kadota" MisV0925 20000505.64875 112C Mis image="Nobuo Ohkura" MisV0925 20000505.65062 113C Mis image="Nobuo Ohkura" Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star MisV0925. It was detected by the PIXY system as one of the candidates of new variable stars from images taken by Ohkura comparing with images taken by Kadota, then confirmed by Yoshida. 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/