Dear colleagues, I am Seiichi Yoshida, working on the MISAO Project. Here I report the magnitude data of variable stars. The magnitude are estimated automatically by the PIXY system from CCD images taken by Seiichiro Kiyota. The magnitude data are also available at the MISAO Project Home Page: http://vsnet.info.waseda.ac.jp/muraoka/members/seiichi/misao/ NSV09699 981011.81922 125Rc Mis NSV09699 981011.82079 123Rc Mis NSV09699 981011.82227 125Rc Mis NSV09699 981011.82380 123V Mis NSV09699 981011.82539 124V Mis NSV09699 981011.82668 124V Mis NSV09699 981011.82867 125V Mis NSV09699 981011.82995 127V Mis NSV09699 981011.83404 126Rc Mis NSV09699 981011.83613 125Rc Mis -- Seiichi Yoshida Muraoka Lab., Waseda University, Japan seiichi@muraoka.info.waseda.ac.jp http://vsnet.info.waseda.ac.jp/muraoka/members/seiichi/index.html