Dear colleagues, New variable star discovery by the MISAO Project (MisV0041). MisV0041 R.A. 17h59m49s.03 Decl. -29o35'40".5 (2000.0) Mag. 12.6C-14.6C = GSC6853.4327 17 59 49.03 -29 35 40.5 12.67 = USNO0600.14864584 17 59 49.054 -29 35 40.29 14.9R 12.4B = IRAS 17566-2935 R.A.=17 59 49.67 Decl.=-29 35 43.7 (57 x 7", p.a.=92) flux(12)=1.67 flux(25)=0.73 flux(60)=<10.31 flux(100)=<108.30 0% variable http://vsnet.info.waseda.ac.jp/muraoka/members/seiichi/misao/data/MisV/MisV0041.gif MisV0041 990408.75863 145C Mis MisV0041 990408.75917 144C Mis MisV0041 990430.73977 146C Mis MisV0041 990520.68250 126C Mis MisV0041 990520.68331 126C 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. V735 Sgr is only 116 arcsec from this star. The data in the GCVS of V735 Sgr is: V735 SGR R.A.=17 59 51.62 Decl.=-29 33 49.5 13.5 - 16.5 mag (P) type:ISB: No evident star exists on our images at this GCVS position. But probably there is a very faint (16 mag or fainter) star at this position. Please see the URL below for the MISAO Project and the PIXY system. http://vsnet.info.waseda.ac.jp/muraoka/members/seiichi/misao/ -- Seiichi Yoshida seiichi@muraoka.info.waseda.ac.jp http://vsnet.info.waseda.ac.jp/muraoka/members/seiichi/index.html