Dear colleagues, We made spectroscopic observations of V893 Sco just recently rediscovered by Kato et al. (submitted to IBVS) by the NTT telescope at ESO on April 18.4 (UT). Then, we confirmed the dwarf novae nature of this star by detecting double-peaked strong emmision lines of Halpha and Hbeta, suggesting V893 Sco to be a high-inclination system. Best regards, Daisaku Nogami, Ronald Mennickent, and Katsura Matsumoto