Photographic observations by TmzV14 by Ymo (bright maximum in 1993) M. Yamamoto reports his previous independent discovery of the variable, presently known as TmzV14. He detected the object in 1993, and reported to the National Astronomical Observatory of Japan. The object was then identified as an IRAS source, and left unreported as a new variable star. The next maximum in 1994 (by Wakuda) only reached mag 12. The 1993 maximum was exceptionally bright one. The total range of variability thus becomes 10.2-(15.6p. Photograpic magnitude estimates by VSOLJ members object YYMMDD(UT) mag code TmzV14 930317.753 <110 Ymo.VSOLJ TmzV14 930319.801 <115 Ymo.VSOLJ TmzV14 930514.617 107 Ymo.VSOLJ TmzV14 930523.551 107 Ymo.VSOLJ TmzV14 930604.533 102 Ymo.VSOLJ Observer's code: Ymo: M. Yamamoto ( Aichi, Japan ) instruments:f200mmPO0 + Tmax400 Seq.:GSC