2010CBET.2588....2P

G. Pignata, Universidad Andres Bello; and G. Folatelli, IPMU, University of Tokyo; on behalf of the Millennium Center for Supernova Science, report on an optical spectrogram (range 355-887 nm) of 2010kt obtained on Dec. 13.14 UT with the SOAR telescope (+ Goodman HTS). The spectrum shows 2010kt to be a normal type-Ia supernova at about two weeks after maximum light. Cross- correlation with a library of supernova spectra using the "Supernova Identification" code (SNID; Blondin and Tonry 2007, Ap.J. 666, 1024) provides good matches with spectra of SNe 1989B, 1994D, and 1996X between +12 and +14 days.