Dear colleagues, New variable star discovery by the MISAO Project (MisV0822). MisV0822 R.A. 16h58m24s.04 Decl. -20o23'36".2 (2000.0) Mag. 11.1C-12.1C Type SR: = USNO-A2.0_0675.17231940 16 58 24.044 -20 23 36.24 12.1R 15.9B = IRAS 16554-2019 R.A.=16 58 22.98 Decl.=-20 23 36.5 (66 x 8", p.a.=96) flux(12)=0.84 flux(25)=0.37 flux(60)=<0.40 flux(100)=<1.54 0% variable http://vsnet.aerith.net/misao/data/MisV/MisV0822.gif MisV0822 19990129.82902 115C Mis MisV0822 19990220.81169 119C Mis MisV0822 19990220.81260 121C Mis MisV0822 19990328.77351 115C Mis MisV0822 19990328.77440 118C Mis MisV0822 19990414.71247 114C Mis MisV0822 19990414.71301 114C Mis MisV0822 19990508.70100 111C Mis MisV0822 19990508.70150 111C Mis MisV0822 19990801.51828 118C Mis MisV0822 19990801.51944 118C Mis MisV0822 20000224.79705 117C Mis MisV0822 20000224.79815 117C 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/