PESSTO spectroscopic classification of optical transients
ATel #10127; C. Barbarino, A. Nyholm, F. Taddia, C. Fremling, J. Sollerman (OKC), J. Lyman (Univ. of Warwick), T.-W. Chen (MPE), C. Inserra, E. Kankare, K. Maguire, S. J. Smartt, K. W. Smith, D. Wright, D. Young (QUB), M. Sullivan (Southampton), S. Valenti (UC Davis), O. Yaron, I. Manulis, (Weizmann), K. C. Chambers, H. Flewelling, M. Huber, T. Lowe. E. Magnier, A. Schulz, C. Waters, R. J. Wainscoat, M. Wilman (IfA, Univ. Hawaii)
on 25 Feb 2017; 16:37 UT
Distributed as an Instant Email Notice Supernovae
Credential Certification: Francesco Taddia (firstname.lastname@example.org)
Subjects: Supernovae, Transient
PESSTO, the Public ESO Spectroscopic Survey for Transient Objects (see Smartt et al. 2015, A&A, 579, 40 http://www.pessto.org ),
reports the following supernova classification. The target was supplied
by Pan-STARRS Survey for Transients (see Chambers et al. 2016, arXiv:1612.05560, and http://pswww.ifa.hawaii.edu ).
The observation was performed on the ESO New Technology Telescope
at La Silla on 2017 February 24, using EFOSC2 and Grism 13 (3985-9315A, 18A resolution).
The classification was done with SNID (Blondin & Tonry, 2007, ApJ, 666, 1024) and GELATO (Harutyunyan et al.,
2008, A&A, 488, 383). The classification spectrum and additional details can be obtained
from http://www.pessto.org (via WISeREP) and the IAU Transient Name Server.
Survey Name | IAU Name | RA (J2000) | Dec (J2000) | Disc. Date | Source | Disc Mag | z | Type | Phase | Notes
PS17bew | SN2017bbq | 11 13 30.67 | +29 40 03.0 | 20170218 | PS1 | 20.1 | 0.046 | II | +36 d | (1)
(1) Red spectrum with narrow Halpha in emission. Best SNID fit to SN IIP 2004dj at +36 d. Other good fits to SN IIn 1998S. Redshift from SDSS.