Electronic Telegram No. 3523 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 2013ck A. J. Drake, S. G. Djorgovski, M. J. Graham, A. Mahabal, and R. Williams, California Institute of Technology; J. L. Prieto, Princeton University; M. Catelan, Pontificia Universidad Catolica de Chile; and S. M. Larson and E. Christensen, Lunar and Planetary Laboratory, University of Arizona, report the Catalina Real-time Transient Survey discovery of an apparent supernova in unfiltered Catalina Sky Survey (CSS) images: SN 2013 UT R.A. (2000.0) Decl. Mag. Offset 2013ck May 8.28 15 24 29.07 +48 32 54.6 17.5 1".1 W, 1".8 N Nothing was visible at this position on a CSS image from Apr. 15.43 UT (limiting mag 20.2). L. Tomasella, S. Benetti, A. Pastorello, E. Cappellaro, P. Ochner, and M. Turatto, Osservatorio Astronomico di Padova, Istituto Nazionale di Astrofisica, report that optical spectroscopy (range 340-820 nm; resolution 1.3 nm), obtained on May 9.04 UT with the Asiago 1.82-m Copernico Telescope (+ AFOSC), shows that 2013ck is a type-Ia supernova at redshift z about 0.049. A good match is found with several normal type-Ia supernovae a few days before maximum light. The expansion velocity, as deduced from the position of the minimum of the Si II 635.5-nm absorption, is about 10300 km/s. The Asiago classification spectra are posted at website URL http://graspa.oapd.inaf.it; classification was made via GELATO (Harutyunyan et al. 2008, A.Ap. 488, 383) and SNID (Blondin and Tonry 2007, Ap.J. 666, 1024). NOTE: These 'Central Bureau Electronic Telegrams' are sometimes superseded by text appearing later in the printed IAU Circulars. (C) Copyright 2013 CBAT 2013 May 13 (CBET 3523) Daniel W. E. Green