Electronic Telegram No. 3242 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 2012fe A. J. Drake, S. G. Djorgovski, M. J. Graham, A. Mahabal, 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. Offset 2012fe Sep. 26.15 17 43 12.18 +36 46 02.5 17.6 2".7 W Additional CSS magnitudes for 2012fe: June 20.29 UT, [20.2; Sept. 6.17, 17.5. L. Tomasella, S. Benetti, E. Cappellaro, P. Ochner, A. Pastorello, M. Turatto, S. Valenti, and M. Fiaschi, Osservatorio Astronomico di Padova, Istituto Nazionale di Astrofisica, report that a low-signal-to-noise spectrogram of 2012fe, obtained on Sept. 28.81 UT with the Asiago 1.82-m Copernico Telescope (+ AFOSC; range 360-820 nm; resolution 1.9 nm), suggests that this is a peculiar type-Ia supernova. Adopting a redshift of about 0.05, cross-correlation with a library of supernova spectra via the "Supernova Identification" code (SNID; Blondin and Tonry 2007, Ap.J. 666, 1024), and best fits with the GELATO software tool (Harutyuyan et al. 2008, A.Ap. 488, 383) using a library of supernovae spectra, show that 2012fe is most similar to several peculiar type-Ia (1991T-like) supernovae about fifteen days after maximum. NOTE: These 'Central Bureau Electronic Telegrams' are sometimes superseded by text appearing later in the printed IAU Circulars. (C) Copyright 2012 CBAT 2012 September 30 (CBET 3242) Daniel W. E. Green