Electronic Telegram No. 3967 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 2014db IN UGC 2988 = PSN J04133846+2528462 Further to CBET 3942, C. Casper, W. Zheng, and A. V. Filippenko, University of California at Berkeley, report the LOSS discovery of a possible supernova in UGC 2988 on unfiltered KAIT images: SN 2014 UT R.A. (2000.0) Decl. Mag. Offset 2014db Aug. 27.52 4 13 38.46 +25 28 46.2 17.1 4".3 W, 12".2 S A finding chart was posted by the discoverers at the following website URL: http://astro.berkeley.edu/~zwk/findingchart/PSN_J04133846+25284620.jpg. The variable was designated PSN J04133846+2528462 when it was posted at the Central Bureau's TOCP webpage and is here designated SN 2014db based on the spectroscopic confirmation reported below. Additional CCD magnitudes for 2014db: Aug. 28.99 UT, 17.6 (G. Masi, P. Catalano, and P. Schmeer; remotely using a 43-cm telescope at Ceccano, Italy; position end figures 38s.48, 46".0); 29.51, 17.1 (KAIT). W. Zheng, K. I. Clubb, and A. V. Filippenko, University of California, Berkeley, report that inspection of a CCD spectrogram (range 350-1000 nm), obtained on Sept. 3.480 UT with the Shane 3-m reflector (+ Kast spectrograph) at Lick Observatory, shows that PSN J04133846+2528462 = SN 2014db is a type-IIP supernova. Cross-correlation with a library of supernova spectra using the "SuperNova Identification" code (SNID; Blondin and Tonry 2007, Ap.J. 666, 1024) indicates a similarity with many type-IIP supernovae about a month after explosion. NOTE: These 'Central Bureau Electronic Telegrams' are sometimes superseded by text appearing later in the printed IAU Circulars. (C) Copyright 2014 CBAT 2014 September 6 (CBET 3967) Daniel W. E. Green