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PESSTO spectroscopic classification of optical transients

ATel #9546; P. James (LJMU), J. Anderson (ESO), L. Short (LJMU), S. Prentice (LJMU), L. Galbany (Univ. de Chile), S. Taubenberger (ESO), C. Inserra (QUB), E. Kankare (QUB), K. Maguire (QUB), S. J. Smartt (QUB), K. W. Smith (QUB), M. Sullivan (Southampton), S. Valenti (UC Davis), O. Yaron (Weizmann), D. Young (QUB), I. Manulis (Weizmann), L. Wyrzykowski,(Warsaw Observatory, Poland)
on 25 Sep 2016; 13:42 UT
Distributed as an Instant Email Notice Supernovae
Credential Certification: Philip James (P.A.James@ljmu.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 OGLE-IV Real-time Transient Search (Wyrzykowski et al., 2014 arxiv:1409.1095; http://ogle.astrouw.edu.pl/ ), and from the ESA Gaia Photometric Science Alerts Team and DPAC (http://gsaweb.ast.cam.ac.uk/alerts). All observations were performed on the ESO New Technology Telescope at La Silla on 2016 September 24th, using EFOSC2 and Grism 13 (3985-9315A, 18A resolution). Classifications were done with SNID (Blondin & Tonry, 2007, ApJ, 666, 1024) 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 
OGLE16dha   |           | 06:32:25.15 | -71:34:04.0 | 20160919   | OGLE   |  18.36   | 0.006 | Ia    |  -1   |  (1) 
Gaia16bif   | SN2016gio | 20:41:57.25 | -40:28:20.4 | 20160916   | Gaia   |  18.81   | 0.094 | Ia    |  +10  |  (2) 

(1) SNID best fit is to Type Ia SN 2007co at z = 0.006 +-0.002
(2) SNID matches Type Ia SN 1994ae at z = 0.094 +-0.004