Dear colleagues, New variable star discovery by the MISAO Project (MisV0990). MisV0990 R.A. 19h40m54s.86 Decl. +18o21'15".2 (2000.0) Mag. 12.1C-13.1C Type SR? = IRAS 19386+1814 R.A.=19 40 55.10 Decl.=+18 21 15.8 (27 x 5", p.a.=71) flux(12)=1.52 flux(25)=0.62 flux(60)=<0.57 flux(100)=<30.68 95% variable = 2MASS 194054.848 +182114.58 (2000.0) 6.685 5.660 5.117 http://vsnet.aerith.net/misao/data/MisV/MisV0990.gif MisV0990 19990715.63538 131C Mis image="KenIchi Kadota" MisV0990 19990715.63604 130C Mis image="KenIchi Kadota" MisV0990 20000525.66708 123C Mis image="Nobuo Ohkura" MisV0990 20000525.66894 121C Mis image="Nobuo Ohkura" Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star MisV0990. 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/