Electronic Telegram No. 3105 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 2012cc IN NGC 4419 = PSN J12265681+1502455 Further to CBET 3037, S. B. Cenko, M. Kandrashoff, W. Li, and A. V. Filippenko report the LOSS discovery of an apparent supernova on unfiltered KAIT images: SN 2012 UT R.A. (2000.0) Decl. Mag. Offset 2012cc Apr. 29.33 12 26 56.81 +15 02 45.5 18.2 7".7 E, 6".7 S The variable was designated PSN J12265681+1502455 when it was posted at the Central Bureau's TOCP webpage and is here designated SN 2012cc based on the spectroscopic confirmation reported below. Additional CCD magnitudes for 2012cc: Apr. 8.41 UT, [18.9 (KAIT); May 11.23, 15.7 (KAIT); 13.509, 14.9 (J. Brimacombe, Cairns, Australia; infrared filter; position end figures 56s.83, 45".8; image posted at http://www.flickr.com/photos/43846774@N02/7192829202/). G. H. Marion and D. Milisavljevic, Harvard-Smithsonian Center for Astrophysics (CfA), on behalf of the CfA Supernova Group, reports that a spectrum (range 340-740 nm) of PSN J12265681+1502455 = 2012cc was obtained on May 13 UT by J. Irwin with the F. L. Whipple Observatory 1.5-m telescope (+ FAST). The object is a heavily reddened type-II supernova. H-alpha produces a broad P-Cyg feature that is similar to that of SN 1987K near maximum brightness (Filippenko 1988, A.J. 96, 1941). The velocity of H-alpha is 13500 km/s, measured at the absorption minimum, but strong reddening suppresses other Balmer series lines. Also similar to SN 1987K, there is evidence for He I in absorption. NOTE: These 'Central Bureau Electronic Telegrams' are sometimes superseded by text appearing later in the printed IAU Circulars. (C) Copyright 2012 CBAT 2012 May 16 (CBET 3105) Daniel W. E. Green