Electronic Telegram No. 2971 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 SUPERNOVAE 2011ju, 2011jv, 2011jw 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; E. C. Beshore and S. M. Larson, Lunar and Planetary Laboratory, University of Arizona; and E. Christensen, Gemini Observatory, report the discovery of three apparent supernovae in unfiltered Catalina Sky Survey (CSS) images: SN 2011 UT R.A. (2000.0) Decl. Mag. Offset 2011ju Dec. 25.35 8 10 43.55 +40 25 29.6 19.2 2" S 2011jv Dec. 27.27 4 48 02.55 - 4 08 22.6 18.8 1" N 2011jw Dec. 27.50 10 47 41.70 + 2 18 15.4 19.3 Additional CSS magnitudes for 2011ju: 2011 Dec. 16.53 UT, [20.1; 30.41, 19.2. Additional CSS magnitudes for 2011jv: 2011 Nov. 28.38, [20.3; 2012 Jan. 2.23, 18.6. Additional CSS magnitudes for 2011jw: 2011 June 6.18, [20.2; 2012 Jan. 2.43, 19.5. J. L. Prieto, Princeton University, reports that optical spectra (range 350-960 nm; resolution 0.7 nm) of SN 2011ju, 2011jv, and 2011jw were obtained with the APO 3.5-m telescope (+ DIS) on Jan. 2 UT, showing all to be type-Ia supernovae. After cross-correlation with a library of supernova spectra using SNID (Blondin and Tonry 2007, Ap.J. 666, 1024), the following redshifts and approximate phases (in days after maximum light) were obtained: 2011ju, 0.103, -2 days; 2011jv, 0.082, +2 days; 2011jw, 0.049, +26 days. NOTE: These 'Central Bureau Electronic Telegrams' are sometimes superseded by text appearing later in the printed IAU Circulars. (C) Copyright 2012 CBAT 2012 January 8 (CBET 2971) Daniel W. E. Green