Electronic Telegram No. 4188 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 2015an IN IC 2367 = PSN J08241502-1846281 L. A. G. Monard, Calitzdorp, Western Cape, South Africa, reports his discovery of an apparent supernova (mag 15.2) on several unfiltered CCD images taken with a 30-cm RCX4000 telescope (+ SBIG ST8-XME camera) at his Klein Karoo Observatory on Sept. 13.15 UT. The new object is located at R.A. = 8h24m15s.02, Decl. = -18d46'28".1 (equinox 2000.0), which is 71" east and 4" north of the center of the type-SBb galaxy IC 2367. The variable was designated PSN J08241502-1846281 when it was posted at the Central Bureau's TOCP webpage and is here designated SN 2015an based on the spectroscopic confirmation reported below. Additional CCD magnitudes for 2015an: Aug. 22.168, [18.5 (Monard); Sept. 15.791, 15.9 (J. Brimacombe, Cairns, Australia; position end figures 15s.07, 28".4; image posted at website URL https://www.flickr.com/photos/43846774@N02/21460420045/); 21.100, 15.1 (Monard); 24.140, 15.0 (Monard); Oct. 4.118, 15.1 (Monard); 6.121, 15.1 (Monard); 8.115, 15.2 (Monard); 13.108, 15.3 (Monard); 17.100, 15.3 (Monard); 18.108, 15.3 (Monard); 25.103, 15.5 (Monard); Nov. 8.083, 15.6 (Monard); 17.094, 15.7 (Monard). G. Hosseinzadeh, S. Valenti, I. Arcavi, D. A. Howell, and C. McCully, Las Cumbres Observatory Global Telescope Network and University of California at Santa Barbara, report that a spectrogram of PSN J08241502-1846281 = SN 2015an, obtained on Sept. 26.7 UT with the robotic FLOYDS instrument (range 320-1000 nm, resolution 2 nm) mounted on the "Faulkes Telescope South" at Siding Spring Observatory, Australia, shows it to be a peculiar type-II supernova. They find a broad H-alpha P-Cyg profile superimposed on a blue continuum. The blue continuum is unusual for a supernova two weeks post- maximum, as is the relatively low H-alpha expansion velocity (about 5000 km/s measured at the proposed host galaxy redshift of z = 0.008; Theureau et al. 1998, A.Ap. Suppl. 130, 333; via NED). Swift ToO observations of this source have been requested. Further follow-up is encouraged. NOTE: These 'Central Bureau Electronic Telegrams' are sometimes superseded by text appearing later in the printed IAU Circulars. (C) Copyright 2015 CBAT 2015 November 18 (CBET 4188) Daniel W. E. Green