Dear colleagues, New variable star discovery by the MISAO Project (MisV0849). MisV0849 R.A. 18h01m40s.53 Decl. -20o16'26".3 (2000.0) Mag. 12.4C-13.2C Type ? = USNO-A2.0_0675.23859821 18 01 40.401 -20 16 24.61 15.5R 19.4B = IRAS 17586-2016 R.A.=18 01 40.31 Decl.=-20 16 23.2 (32 x 6", p.a.=90) flux(12)=7.64 flux(25)=4.65 flux(60)=<3.11 flux(100)=<31.20 5% variable http://vsnet.aerith.net/misao/data/MisV/MisV0849.gif MisV0849 19990408.74544 131C Mis MisV0849 19990408.74600 131C Mis MisV0849 19990430.75147 131C Mis MisV0849 19990430.75190 132C Mis MisV0849 19990831.55657 125C Mis MisV0849 19990831.55773 124C Mis MisV0849 19990923.42338 126C Mis MisV0849 19990923.42427 127C Mis MisV0849 20000224.82436 124C Mis MisV0849 20000224.82494 124C Mis It was detected by the PIXY system as one of the candidates of new variable stars from images taken by KenIchi Kadota, Ageo City, Saitama, Japan, then confirmed by Seiichi Yoshida. The magnitude are measured automatically by the PIXY system. Image observers' names are noted after "Mis", except for ones taken by KenIchi Kadota. 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/