Dear colleagues, I am Seiichi Yoshida, working on the MISAO Project. Here I report the magnitude data of MISAO new variable stars. The magnitude are estimated automatically by the PIXY system from CCD images taken by KenIchi Kadota, Ageo City, Japan. The magnitude data are also available at the MISAO Project Home Page: http://vsnet.info.waseda.ac.jp/muraoka/members/seiichi/misao/ The first variable star, MisV0001, faded out and I could not find the image. MisV0003 keeps fading and updated the minimum magnitude. MisV0004 keeps fading since the discovery and updated the minimum magnitude. Because the magnitude range becomes larger than 2.5 mag, I judged the type as M:. MisV0012 keeps fading since the discovery and updated the minimum magnitude. MisV0017 keeps fading and updated the minimum magnitude. Because the magnitude range becomes larger than 2.5 mag, I judged the type as M:. MisV0030 passed the peak and turned to be fading. MisV0001 990604.61503 <165C Mis MisV0001 990604.61567 <165C Mis MisV0001 990604.61653 <165C Mis MisV0003 990604.61503 136C Mis MisV0003 990604.61567 136C Mis MisV0003 990604.61653 137C Mis MisV0004 990604.61503 148C Mis MisV0004 990604.61567 144C Mis MisV0004 990604.61653 145C Mis MisV0012 990520.68435 141C Mis MisV0012 990520.68480 139C Mis MisV0013 990520.68435 <139C Mis MisV0013 990520.68480 <140C Mis MisV0016 990520.68435 <139C Mis MisV0016 990520.68480 <140C Mis MisV0017 990520.68435 141C Mis MisV0017 990520.68480 138C Mis MisV0025 990520.68435 <139C Mis MisV0025 990520.68480 <140C Mis MisV0026 990520.68435 <139C Mis MisV0026 990520.68480 <140C Mis MisV0030 990520.68435 141C Mis MisV0030 990520.68480 146C Mis MisV0035 990520.68435 <150C Mis MisV0035 990520.68480 <150C Mis MisV0036 990520.68435 <139C Mis MisV0036 990520.68480 <140C Mis -- Seiichi Yoshida seiichi@muraoka.info.waseda.ac.jp http://vsnet.info.waseda.ac.jp/muraoka/members/seiichi/index.html