Electronic Telegram No. 4180 Central Bureau for Astronomical Telegrams Mailing address: 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 2015ag IN IC 43 = PSN J00422186+2938415 Paolo Campaner reports the discovery of an apparent supernova (mag 19.1) on three 75-s unfiltered CCD exposures (limiting magnitude 20.0) obtained on Aug. 6.092 UT with a 0.4-m f/5.5 reflector at Ponte di Piave, Italy, in the course of the Italian Supernovae Search Project. The new object is located at R.A. = 0h42m21s.86, Decl. = +29d38'41".5 (equinox 2000.0), which is 1" west and 12" north of the center of IC 43. The variable was designated PSN J00422186+2938415 when it was posted at the Central Bureau's TOCP webpage and is here designated SN 2015ag based on the spectroscopic confirmation reported below. SN 1973U also appeared on IC 43 (cf. IAUC 2620). Additional CCD magnitudes for 2015ag: Aug. 7.095, 19.0 (Campaner); 8.725, 20.8 (J. Brimacombe, Cairns, Australia; position end figures 21s.96, 40".9; images posted at URL https://www.flickr.com/photos/43846774@N02/20337212839/); 9.104, 19.2 (Campaner); 11.779, 20.4 (Brimacombe; position end figures 21s.96, 41".0); 13.094, 18.9 (G. Masi; remotely using a 43-cm telescope at Ceccano, Italy; position end figures 21s.93, 40".7). G. Terreran, S. Benetti, E. Cappellaro, N. Elias-Rosa, P. Ochner, A. Pastorello, L. Tartaglia, L. Tomasella, and M. Turatto, Osservatorio Astronomico di Padova, Istituto Nazionale di Astrofisica, report that an optical spectrogram (range 340-820 nm; resolution 1.4 nm) of PSN J00422186+2938415 = SN 2015ag, obtained on Aug. 11.05 UT with the Asiago 182-cm Copernico Telescope (+ AFOSC) in the framework of the Asiago Transient Classification Program (Tomasella et al. 2014, A.N. 335, 841), shows that this a type-Ic supernova. Assuming a redshift z = 0.0162 for the host galaxy, IC 43 (Huchra at al. 1999, Ap.J. Supple. 121, 287; via NED), a good match is found with type-Ic supernovae around two-three months post-maximum. Classification was done with GELATO (Harutyunyan et al. 2008, A.Ap. 488, 383) and SNID (Blondin and Tonry 2007, Ap.J. 666, 1024). The Asiago classification spectra are posted at URL http://sngroup.oapd.inaf.it. NOTE: These 'Central Bureau Electronic Telegrams' are sometimes superseded by text appearing later in the printed IAU Circulars. (C) Copyright 2015 CBAT 2015 November 16 (CBET 4180) Daniel W. E. Green