Electronic Telegram No. 2655 Central Bureau for Astronomical Telegrams INTERNATIONAL ASTRONOMICAL UNION CBAT Director: Daniel W. E. Green; Hoffman Lab 209; Harvard University; 20 Oxford St.; Cambridge, MA 02138; U.S.A. e-mail: cbatiau@eps.harvard.edu (alternate cbat@iau.org) URL http://www.cbat.eps.harvard.edu/index.html Prepared using the Tamkin Foundation Computer Network SUPERNOVA 2011ac IN UGC 4552 = PSN J08432216+1043476 Further to CBET 2651, P. Blanchard, M. Mason, S. B. Cenko, W. Li, and A. V. Filippenko report the LOSS discovery of an apparent supernova on unfiltered KAIT images: SN 2011 UT R.A. (2000.0) Decl. Mag. Offset 2011ac Feb. 11.29 8 43 22.16 +10 43 47.6 17.7 11".2 E, 13".9 N This object was given the provisional designation PSN J08432216+1043476 when posted on the Central Bureau's TOCP webpage. Additional (presumed unfiltered CCD) magnitudes for 2011ac: Feb. 2.31 UT, [19.2 (KAIT); 12.118, 18.1 (R. A. Koff, Bennett, CO, U.S.A.; position end figures 22s.12, 48".1); 12.29, 17.8 (KAIT). P. A. Milne, University of Arizona; and S. B. Cenko, University of California, Berkeley, report that inspection of a CCD spectrum (range 400-830 nm), obtained on Feb. 13 UT with the 2.3-m Bok telescope (+ Boller and Chivens spectrograph), shows that 2011ac is a type-Ia supernova. After removal of the host-galaxy recession velocity of 14030 km/s (Falco et al. 1999, PASP 111, 438; via NED), they find the absorption minimum of the Si II 635.5-nm line to be blueshifted by about 12000 km/s. Cross-correlation with a library of supernova spectra using the "SuperNova IDentification" code (SNID; Blondin and Tonry 2007, Ap.J. 666, 1024) indicates that 2011ac is a normal type-Ia supernova shortly before maximum light. NOTE: These 'Central Bureau Electronic Telegrams' are sometimes superseded by text appearing later in the printed IAU Circulars. (C) Copyright 2011 CBAT 2011 February 14 (CBET 2655) Daniel W. E. Green