Electronic Telegram No. 1014 Central Bureau for Astronomical Telegrams INTERNATIONAL ASTRONOMICAL UNION M.S. 18, Smithsonian Astrophysical Observatory, Cambridge, MA 02138, U.S.A. IAUSUBS@CFA.HARVARD.EDU or FAX 617-495-7231 (subscriptions) CBAT@CFA.HARVARD.EDU (science) URL http://www.cfa.harvard.edu/iau/cbat.html SUPERNOVAE 2007ge AND 2007gh Further to CBET 1013, the "Nearby Supernova Factory" collaboration (G. Rigaudier and E. Pecontal, Centre de Recherche Astronomique de Lyon; C. Buton, Y. Copin, E. Gangler, and G. Smadja, Institut de Physique Nucleaire de Lyon; P. Antilogus, R. Pain, R. Pereira, and C. Wu, Laboratoire de Physique Nucleaire et de Haute Energies de Paris; G. Aldering, C. Aragon, S. Bailey, S. Bongard, M. Childress, S. Loken, P. Nugent, S. Perlmutter, K. Runge, R. C. Thomas, and B. A. Weaver, Lawrence Berkeley National Laboratory, Berkeley; C. Baltay, A. Bauer, D. Rabinowitz, and R. Scalzo, Yale University; D. Birchall, Institute for Astronomy, University of Hawaii, Hilo; and J. Holtzman, New Mexico State University, Las Cruces) reports the discovery of a type-II supernova (mag R = 19.1) in images obtained on July 29 UT using the QUEST-II camera on the Palomar Oschin 1.2-m Schmidt telescope, operated by the Palomar-QUEST Consortium. SN 2007gh is located at R.A. = 2h10m31s.08, Decl. = +2o19'59".3 (equinox 2000.0). A spectrum (range 320-1000 nm) of 2007gh, obtained on Aug 1.6 with the SuperNova Integral Field Spectrograph (SNIFS) on the University of Hawaii 2.2-m telescope, indicates that the supernova appears to be a few months old, with strong hydrogen Balmer emission features; an approximate redshift of z = 0.02 is derived by measuring the peak of the observed H-alpha feature. Also, a SNIFS spectrum of 2007ge (cf. CBET 1012), obtained on Aug. 1.5 UT, indicates that it is a type-Ia supernova, a few days past maximum. NOTE: These 'Central Bureau Electronic Telegrams' are sometimes superseded by text appearing later in the printed IAU Circulars. (C) Copyright 2007 CBAT 2007 August 1 (CBET 1014) Daniel W. E. Green