Electronic Telegram No. 4057 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 2014ed Tomoki Morokuma, Institute of Astronomy, University of Tokyo; Nozomu Tominaga, Emiko Matsumoto, and Takumi Shibata, Konan University; Masaomi Tanaka, National Astronomical Observatory of Japan; and Satoru Fukuda, Hyogo, Japan -- on behalf of the Kiso Supernova Survey (KISS) collaboration -- report the discovery of an apparent supernova (mag 19.5) on a g-band CCD image (limiting mag 20.9) taken on 2014 Nov. 21.76 UT with the Kiso Wide Field Camera (field-of-view 2.1 deg x 2.1 deg) on the 1.05-m Kiso Schmidt telescope. The new object is located at R.A. = 9h29m13s.75, Decl. = +22d34'36".4 (equinox 2000.0), which is 1".2 east and 0".3 south of the center of the galaxy SDSS J092913.67+223436.6. Tomoki Morokuma, Mitsuru Kokubo, Kazuma Mitsuda, Yasuhito Hashiba, Mamoru Doi, Shigeyuki Sako, Yuki Kikuchi, Hidenori Takahashi, and Ken Tateuchi, University of Tokyo; Hanindyo Kuncarayakti, Millennium Institute of Astrophysics, Chile; Makoto Watanabe and Hikaru Nakao, Hokkaido University; and Yoichi Itoh, Kumiko Morihana, Satoshi Honda, Yuhei Takagi, and Jun Takahashi, University of Hyogo, report that low-resolution optical spectra (range 400-1000 nm) of 2014ed were obtained on 2014 Nov. 23.82 and 27.73 UT with the Line Imager and Slit Spectrograph (Hashiba et al. 2014, SPIE 9147, 2) on the 2.0-m Nayuta telescope at Nishi-Harima Observatory. Cross-correlation with a library of supernova spectra via the SNID code (Blondin and Tonry 2007, Ap.J. 666, 1024) shows a best fit with type-Ia supernovae at z = 0.15 around or a few days before maximum. NOTE: These 'Central Bureau Electronic Telegrams' are sometimes superseded by text appearing later in the printed IAU Circulars. (C) Copyright 2015 CBAT 2015 January 25 (CBET 4057) Daniel W. E. Green