Electronic Telegram No. 1199
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)
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SUPERNOVA 2007uz IN PGC 34755
     F. Olivares, University of Chile; and N. Morrell, Las Campanas
Observatory, on behalf of the Carnegie Supernova Project and the Millenium
Center for Supernova Studies, report that a spectrum (range 350-950 nm) of
2007uz (cf. CBET 1192), obtained on Jan. 4.92 UT with the European Southern
Observatory 3.6-m telescope (+ EFOSC) at La Silla, shows this to be a
type-Ia supernova several weeks past maximum light.  Assuming for the host
galaxy the NED recession velocity of 8917 km/s (da Costa et al. 1987, A.J.
93, 1338) the 'superfit' comparison tool (Howell et al. 2005, Ap.J. 634,
1190) provides excellent matches to the spectrum of 1998bu between 30 and 40
days after maximum light.


NOTE: These 'Central Bureau Electronic Telegrams' are sometimes
      superseded by text appearing later in the printed IAU Circulars.

                         (C) Copyright 2008 CBAT
2008 January 7                   (CBET 1199)              Daniel W. E. Green