Electronic Telegram No. 2975 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 2012A IN NGC 3239 Y. Cao, California Institute of Technology; M. M. Kasliwal, Observatories of the Carnegie Institution for Science and Princeton University; G. Wallerstein and A. Ritchey, University of Washington; and D. A. Howell, Las Cumbres Observatory Global Telescope and University of California at Santa Barbara, on behalf of a large collaboration, report that they obtained a low-resolution spectrum of SN 2012A (cf. CBET 2974) on Jan. 10.275 UT with the Dual Imaging Spectograph on the ARC 3.5-m telescope at Apache Point Observatory. The presence of a blue continuum and P-Cyg Balmer features allow them to classify 2012A as a type-II supernova. The minimum of the H-alpha absorption is blue-shifted by 9000 km/s. Rupak Roy, Aryabhatta Research Institute of Observational Sciences, Nainital; and Sayan Chakraborti, Tata Institute of Fundamental Research, Mumbai, on behalf of a larger collaboration, report that SN 2012A is a type-IIP supernova. Medium-resolution slit spectroscopy (range 350-750 nm) was acquired at the IUCAA Girawali Observatory on Jan. 10, showing broad H_alpha and H_beta features. With the help of the SNID code (Blondin and Tonry 2007, Ap.J. 666, 1024), they find the spectra to be most similar to that of the type-IIP supernova 2004et at age 1.9 days before maximum (age from explosion 14.2 days). The spectra are also similar to SN 2008in (also a type-IIP event; Chakraborti et al. 2008, CBET 1638) before maximum light. NOTE: These 'Central Bureau Electronic Telegrams' are sometimes superseded by text appearing later in the printed IAU Circulars. (C) Copyright 2012 CBAT 2012 January 12 (CBET 2975) Daniel W. E. Green