Dear colleagues, I am Seiichi Yoshida, working on the MISAO Project. Here I report the magnitude data of variable stars. The magnitude are measured 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/ AQLHP 19990414.76369 111C Mis AQLHP 19990724.52014 130C Mis AQLHP 19990724.52059 130C Mis AQLHQ 19980620.68597 102C Mis AQLHQ 19990414.76369 113C Mis AQLHQ 19990724.52014 106C Mis AQLHQ 19990724.52059 106C Mis HERV585 19990429.71163 137C Mis HERV585 19990429.71233 136C Mis HERV585 19990429.71279 137C Mis HERV585 19990707.66400 143C Mis HERV585 19990707.66444 145C Mis HS1411 19990220.84734 117C Mis HS1411 19990220.84824 117C Mis HS1411 19990414.75911 112C Mis HS1411 19990414.75954 112C Mis HS1411 19990508.71193 107C Mis blending HS1411 19990508.71236 109C Mis HS1411 19990724.51391 114C Mis HS1411 19990724.51481 114C Mis SCTEI 19990414.76537 125C Mis SCTEI 19990414.76580 125C Mis SCTEI 19990508.72023 130C Mis SCTEI 19990508.72066 131C Mis SCTEI 19990724.52280 143C Mis SCTEI 19990724.52324 143C Mis SCTV347 19990414.76645 120C Mis SCTV347 19990414.76689 119C Mis SCTV347 19990508.72201 122C Mis SCTV347 19990508.72244 122C Mis SCTV347 19990724.52435 139C Mis -- Seiichi Yoshida seiichi@muraoka.info.waseda.ac.jp http://vsnet.info.waseda.ac.jp/muraoka/members/seiichi/index.html