NSV15573: confirmation of large-amplitude variation by Toa Akira Takao (Kita-kyushu, Japan) reports the discovery of large-amplitude variation in NSV15573. NSV15573 = IRAS02433+6345 024321.0 +634542 (1950.0) F12=20.89 F25=17.37 F60=2.29 F100=3.98L VAR=99 LRS=29 blue, 10micron (silicate) emission, strength=9 IIIa: variable star with more evolved O-rich c.s. shell = 024724.6 +635814 (2000.0) IRAS02433+6345 20.080 16.780 2.386 3.997L 99% 3(LRS) = 024724.6 +635814 (2000.0) SSC02433+6345 20.080 16.780 2.386 3.997L This observation supports that the star is a large-amplitude Mira star. CCD magnitude estimates by VSOLJ members object YYYYMMDD(UT) mag code NSV15573 20001105.585 <146C Toa.VSOLJ NSV15573 20001201.689 <146C Toa.VSOLJ NSV15573 20011013.594 125C Toa.VSOLJ NSV15573 20011013.647 125C Toa.VSOLJ magnitude compared to GSC4055.382, GSC4055.936, GSC4055.1474 Observer's code: Toa: Akira Takao (Kita-kyushu, Japan) instruments:f200mm F4 Telephotolens+ST-8,unfiltered Relayed from Akira Takao <drtakao@bronze.ocn.ne.jp>