[IAUC] CBET 2717: 20110511 : SUPERNOVA 2011cg
quai en eps.harvard.edu
quai en eps.harvard.edu
Mie Sep 14 16:18:54 ART 2011
Electronic Telegram No. 2717
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 en eps.harvard.edu (alternate cbat en iau.org)
URL http://www.cbat.eps.harvard.edu/index.html
Prepared using the Tamkin Foundation Computer Network
SUPERNOVA 2011cg
A. J. Drake, S. G. Djorgovski, A. Mahabal, M. J. Graham, and R. Williams,
California Institute of Technology; J. L. Prieto, Carnegie Observatories;
M. Catelan, Pontificia Universidad Catolica de Chile; E. C. Beshore and S. M.
Larson, Lunar and Planetary Laboratory, University of Arizona; and E.
Christensen, Gemini Observatory, report the Catalina Real-time Transient
Survey's discovery of an apparent supernova in unfiltered Catalina Sky Survey
images:
SN 2011 UT R.A. (2000.0) Decl. Mag. Offset
2011cg Apr. 14.33 14 59 09.25 + 7 18 04.2 15.7 2" W, 1" S
G. H. Marion, Harvard-Smithsonian Center for Astrophysics (CfA), on
behalf of the CfA Supernova Group, report that a spectrum (range 340-740 nm)
of 2011cg was obtained on May 5 UT by P. Berlind with the F. L. Whipple
Observatory 1.5-m telescope (+ FAST). Cross-correlation with a library of
supernova spectra using the "Supernova Identification" code (SNID; Blondin
and Tonry 2007, Ap.J. 666, 1024) shows that 2011cg is a type-Ia supernova
about two weeks after maximum light.
NOTE: These 'Central Bureau Electronic Telegrams' are sometimes
superseded by text appearing later in the printed IAU Circulars.
(C) Copyright 2011 CBAT
2011 May 11 (CBET 2717) Daniel W. E. Green
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