SALT spectroscopic classification of PS16eot (= SN 2016hfb) as a type-II supernova
ATel #9657; S. W. Jha, K. Dettman (Rutgers), Y.-C. Pan, R. J. Foley (UCSC), A. Rest (STScI), D. Scolnic (Chicago/KICP), B. Miszalski, E. Romero Colmenero (SALT/SAAO)
on 20 Oct 2016; 21:12 UT
Distributed as an Instant Email Notice Supernovae
Credential Certification: Saurabh Jha (saurabh@physics.rutgers.edu)
Subjects: Optical, Supernovae
We obtained SALT (+RSS) spectroscopy of PS16eot (= SN 2016hfb) on
2016 Oct 19.9 UT, covering the wavelength range 340-920 nm. Narrow
emission lines confirm the redshift of the host galaxy UGC 2372 at z =
0.026 (Haynes et al. 1997, AJ, 113, 1197; via NED).
Cross-correlation of the spectrum with a supernova template library
using SNID (Blondin & Tonry 2007, ApJ, 666, 1024) shows PS16eot is a
type-II supernova approximately one week past maximum light. A good
SNID match is obtained with the type-IIP SN 2004et at +6 days. The
expansion velocity for PS16eot, measured to the trough of the H-beta
line, is approximately 8000 km/s.
Our spectrum is posted on the Transient Name Server
SN 2016hfb page.
PS16eot was discovered as part of the
Pan-STARRS Survey for Transients (Huber et al. 2015, ATel
#7153). Information on all PSST objects is available at http://star.pst.qub.ac.uk/ps1threepi/