Electronic Telegram No. 3080 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 2012bp Vladimir Lipunov reports the discovery of a possible supernova (mag 15.5) on three unfiltered CCD images (limiting mag 18.8) taken with the MASTER II dual 40-cm telescope (+ Apogee CCD Alta U16m camera; field-of-view 2 deg x 4 deg) at the Tunka observatory as part of the MASTER auto-detection system (see website URL (http://observ.pereplet.ru) on Mar. 24.852 UT. The new object is located at R.A. = 16h18m12s.44, Decl. = +36d28'52".8 (equinox 2000.0). Nothing is visible at this position on a reference image taken on 2011 June 28.677 (limiting mag 20.0). The discovery and reference images are available at website URL http://master.sai.msu.ru/static/OT/161812.44362852.8.png. A. Pastorello, S. Benetti, E. Cappellaro, M. Fiaschi, P. Ochner, L. Tomasella, M. Turatto, and S. Valenti, Osservatorio Astronomico di Padova, Istituto Nazionale di Astrofisica, report that a spectrogram of 2012bp, obtained on Mar. 27.13 UT with the Asiago 1.82-m Copernico Telescope (+ AFOSC; range 340-820 nm; resolution 2.4 nm), suggests that it is a type-Ia supernova. Adopting for the host galaxy a redshift z = 0.02829 (SDSS 2004, via NED) the comparison with a library of supernovae spectra via GELATO (Harutyuyan et al. 2008, A.Ap. 488, 383) shows that 2012bp is a type-Ia event similar to SN 2003du (Stanishev et al. 2007, A.Ap. 469, 645) close to B-band maximum light. The expansion velocity deduced from the Si II 635.5-nm minimun is about 10800 km/s. NOTE: These 'Central Bureau Electronic Telegrams' are sometimes superseded by text appearing later in the printed IAU Circulars. (C) Copyright 2012 CBAT 2012 March 31 (CBET 3080) Daniel W. E. Green