Confirmation and Spectroscopic Classification of MASTER SN candidate in PGC066672

Details Confirmation and Spectroscopic Classification of MASTER SN candidate in PGC066672 Confirmation and Spectroscopic Classification of MASTER SN candidate in PGC066672

Nov 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010atel.2992....1m&link_type=abstract

The Astronomer's Telegram, #2992

Astronomy and Astrophysics

Astronomy

Optical, Supernovae

Scientific paper

Inspection of CCD spectra (range 440-780 nm), obtained on Oct 30 UT with the 2.4-m Hiltner telescope (+ MKIII) at MDM Observatory, shows that the possible supernova in PCG066672 (ATel #2973) is a type-Ia event almost three weeks past maximum light. Comparison with a library of supernova spectra using the "SuperNova Identification" code (SNID; Blondin and Tonry 2007, ApJ, 666, 1024) provides a good match with the normal type-Ia SN 2002bo 19 days past maximum.

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