Electronic Telegram No. 3297 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 2012gh A. A. Mahabal, A. J. Drake, S. G. Djorgovski, M. J. Graham, and R. Williams, California Institute of Technology; J. L. Prieto, Princeton University; M. Catelan, Pontificia Universidad Catolica de Chile; and S. M. Larson and E. Christensen, Lunar and Planetary Laboratory, University of Arizona, report the discovery of an apparent supernova in unfiltered Catalina Sky Survey (CSS) images: SN 2012 UT R.A. (2000.0) Decl. Mag. 2012gh Oct. 26.09 16 46 52.49 +56 51 05.4 18.0 Nothing was visible at this position on a CSS image from June 22.27 UT (limiting mag 19.0). Photometric magnitudes for 2012gh, obtained with the Palomar 1.5-m telescope (+ Gunn filters): Nov. 5.11, g = 18.1, r = 17.8, i = 17.5, z = 17.0. L. Tomasella, S. Benetti, E. Cappellaro, A. Pastorello, M. Turatto, and M. Fiaschi, Osservatorio Astronomico di Padova, Istituto Nazionale di Astrofisica, report that optical spectroscopy (range 340-820 nm; resolution 1.3 nm), obtained on Nov. 5.78 UT with the Asiago 1.82-m Copernico Telescope (+ AFOSC), shows that 2012gh is a type-Ic supernova at a redshift z, about, 0.07. The best match was found with the type-Ic supernova 2007gr (Tanaka et al. 2008, Ap.J. 689, 1191; Valenti et al. 2008, Ap.J. 673, L155) some days after maximum. The Asiago classification spectra are posted at website URL http://graspa.oapd.inaf.it; classification was made via GELATO (Harutyunyan et al. 2008, A.Ap. 488, 383) and SNID (Blondin and Tonry 2007, Ap.J. 666, 1024). NOTE: These 'Central Bureau Electronic Telegrams' are sometimes superseded by text appearing later in the printed IAU Circulars. (C) Copyright 2012 CBAT 2012 November 13 (CBET 3297) Daniel W. E. Green