Electronic Telegram No. 2702 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 2011br IN NGC 5881 = PSN J15062020+6259006 Further to CBET 2678, M. Mason, K. Lin, S. B. Cenko, W. Li, and A. V. Filippenko report the LOSS discovery of an apparent supernova on unfiltered KAIT images: SN 2011 UT R.A. (2000.0) Decl. Mag. Offset 2011br Apr. 9.50 15 06 20.20 +62 59 00.6 18.2 5".2 W, 10".0 S This variable was designated PSN J15062020+6259006 when posted on the Central Bureau's TOCP webpage and is here designated SN 2011br based on the spectroscopic report below. Additional CCD magnitudes for 2011br: Mar. 10.54 UT, [19.3 (KAIT); Apr. 10.48, 18.4 (KAIT); 11.133, 18.2 (Joseph Brimacombe, Cairns, Australia; remotely using a 51-cm RCOS telescope + STL11K camera + red filter at New Mexico Skies Observatory, Mayhill, NM, U.S.A.; position end figures 20s.17, 00".6); 17.245, 17.8 (Brimacombe). Brimacombe's Apr. 11 image is posted at http://www.flickr.com/photos/43846774@N02/5610004688/; his image from Apr. 17 is posted at http://www.flickr.com/photos/43846774@N02/5629808506/. J. M. Silverman and A. V. Filippenko, University of California,Berkeley, report that inspection of a fairly noisy CCD spectrum (range 340-1000 nm), obtained by A. Sonnenfeld (University of California, Santa Barbara) on Apr. 15 UT with the 3-m Shane reflector (+ Kast) at Lick Observatory, shows that PSN J15062020+6259006 = SN 2011br is likely a type-Ib supernova. The host galaxy is at a redshift of 0.0221 (calculated from narrow emission lines in the spectrum). NOTE: These 'Central Bureau Electronic Telegrams' are sometimes superseded by text appearing later in the printed IAU Circulars. (C) Copyright 2011 CBAT 2011 April 20 (CBET 2702) Daniel W. E. Green