[IAUC] CBET 1726: 20090319 : SUPERNOVA 2009ap IN ESO 138-27

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                                                  Electronic Telegram No. 1726
Central Bureau for Astronomical Telegrams
INTERNATIONAL ASTRONOMICAL UNION
M.S. 18, Smithsonian Astrophysical Observatory, Cambridge, MA 02138, U.S.A.
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SUPERNOVA 2009ap IN ESO 138-27
     M. Stritzinger, N. Morrell, and F. Salgado, on behalf of the Carnegie
Supernova Project, report they obtained a spectrogram (range 402.7-1011 nm)
of 2009ap (cf. CBET 1712), obtained on Mar. 16.1 UT with the Magellan I BAADE
(+ IMACS) telescope, appears to be that of a type-Ic supernova several weeks
past maximum.  Adopting a host-galaxy recession velocity of 6230 km/s (H I
Parkes All-Sky Survey Final Catalog; Wong et al. 2006, MNRAS 371, 1855) for
the host galaxy (ESO 138-27), Fe II (rest 516.9 nm) and O I (rest 777.4 nm)
are measured to be blue-shifted by roughly 5600 and 6700 km/s, respectively.


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                         (C) Copyright 2009 CBAT
2009 March 19                    (CBET 1726)              Daniel W. E. Green



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