2005CBET..122....1S

B. Schmidt and M. Salvo, Australian National University (ANU), report that a spectrogram (range 320-1050 nm) of SN 2005at (cf. CBET 119), obtained on Mar. 19.77 UT with the ANU 2.3-m telescope (+ DBS), reveals it to be a type-Ic supernova resembling SN 1994I at approximately 2 weeks past maximum light. The relatively red spectrum is dominated by broad P-Cyg profiles of the Ca II infrared triplet, Na D line, and what appears to be He I 1083-nm.