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PESSTO spectroscopic classification of optical transients

ATel #9706; M. Pursiainen, G. Dimitriadis, R. E. Firth, R. Cartier (Southampton), J. Lyman (Univ. of Warwick), C. Inserra, E. Kankare, K. Maguire, S. J. Smartt, K. W. Smith (QUB), M. Sullivan (Southampton), S. Valenti (UC Davis), O. Yaron (Weizmann), D. Young (QUB), I. Manulis (Weizmann), J. Tonry, B. Stalder, L. Denneau., A. Heinze, A. Sherstyuk (IfA, Univ. of Hawaii), A. Rest (STScI), L. Wyrzykowski (Warsaw Observatory, Poland)
on 3 Nov 2016; 17:31 UT
Distributed as an Instant Email Notice Supernovae
Credential Certification: Robert Firth (r.firth@soton.ac.uk)

Subjects: Optical, Supernovae

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 classifications. Targets were supplied by the ATLAS survey, see Tonry et al. (2011 PASP, 123, 58) and Tonry et al. (ATEL #8680), the ESA Gaia Photometric Science Alerts Team and DPAC (http://gsaweb.ast.cam.ac.uk/alerts) and OGLE-IV Real-time Transient Search (Wyrzykowski et al., 2014 arxiv:1409.1095; http://ogle.astrouw.edu.pl/ ). All observations were performed on the ESO New Technology Telescope at La Silla on 2016 Nov 02, using EFOSC2 and Grism 13 (3985-9315A, 18A resolution). Classifications were done with SNID (Blondin & Tonry, 2007, ApJ, 666, 1024), SuperFit (Howell et al., 2005, ApJ, 634, 1190) and GELATO (Harutyunyan et al., 2008, A&A, 488, 383). Classification spectra 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 
ATLAS16dqn  | SN2016hqh | 07 57 05.80 | +23 08 55.3 |  20161024  | ATLAS  |   17.28  | 0.054 |  Ia  | +10d   | 
ATLAS16drn  | SN2016hhv | 23 35 48.47 | +20 42 31.6 |  20161024  | ATLAS  |   19.1   | 0.062 |  Ia  | -2d    | 
Gaia16bnf   | SN2016gxq	| 08 17 26.83 | +21 41 25.5 |  20160920  | Gaia   |   18.2   | 0.015 |  Ia  | >+100d | (1) 
OGLE16fbw   |           | 06 27 54.95 | -70 24 55.1 |  20161023  | OGLE   |   19.57  | 0.099 |  Ia  | +10d   | 

(1) - Best fit is to nebular spectrum of SN2002fk at a phase of +119 days.