Electronic Telegram No. 4184 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 2015ak IN ESO 108-21 = PSN J22151967-6532534 Peter Marples, Loganholme, Queensland, Australia, reports the discovery of an apparent supernova (mag 16.0) on an unfiltered image (limiting red mag 17.5) taken on Aug. 18.54 UT with a 30-cm Meade LX200ACF f/7 reflector; the new object is located at R.A. = 22h15m19s.67, Decl. = -65d32'53".4 (equinox 2000.0), which is 18" east and 6" north of the center of ESO 108-21. Nothing is visible at this position on Digitized Sky Survey red and infrared images (limiting red mag 19). The variable was designated PSN J22151967-6532534 when it was posted at the Central Bureau's TOCP webpage and is here designated SN 2015ak based on the spectroscopic confirmation reported below. Additional CCD magnitudes for 2015ak: Aug. 2.57, [17.5 (Marples); 10.435, 18.7 (S. Parker, Canterbury, New Zealand; limiting mag 19; pre-discovery image); 18.55, 16.0 (G. Bock, Runaway Bay, Gold Coast, Qld., Australia); 19.729, 17.0 (J. Brimacombe, Cairns, Australia; position end figures 19s.52, 53".6; image posted at https://www.flickr.com/photos/43846774@N02/20732971441/). G. Hosseinzadeh, I. Arcavi, S. Valenti, C. McCully, and D. A. Howell, Las Cumbres Observatory Global Telescope Network and University of California, Santa Barbara, report that a spectrogram of PSN J22151967-6532534 = SN 2015ak, obtained on Aug. 19.4 UT with the FLOYDS robotic spectrograph (range 320-1000 nm, resolution 2 nm) mounted on the 2-m "Faulkes Telescope South" at Siding Spring Observatory, Australia, shows it to be a type-Ia supernova. Using SNID (Blondin and Tonry 2007, Ap.J. 666, 1024), they find a good fit to the normal type-Ia supernova 1999ee at nine days before maximum light at the redshift of the proposed host galaxy (z = 0.010; Ramella et al. 1996, A.Ap. 312, 745; via NED). NOTE: These 'Central Bureau Electronic Telegrams' are sometimes superseded by text appearing later in the printed IAU Circulars. (C) Copyright 2015 CBAT 2015 November 17 (CBET 4184) Daniel W. E. Green