Support ATel At Patreon

[ Previous | Next | ADS ]

Pessto spectroscopic classification of optical transients

ATel #5683; P.-F. Leget (LPC Clermont), L. Le Guillou, M. Fleury, S. Baumont, C. Balland (LPNHE), A. Pastorello, S. Benetti, (Padova), C. Inserra, S. Smartt, K. Smith, D. Young (QUB), M. Sullivan (Southampton), S. Taubenberger (MPA), S. Valenti (LCOGT), M. Fraser (IoA), O. Yaron, I. Manulis, A. Gal-Yam, (Weizmann), C. Knapic, R. Smareglia, M. Molinaro (Trieste), C. Baltay, N. Ellman, E. Hadjiyska, R. McKinnon, D. Rabinowitz, E. S. Walker (Yale University), U. Feindt, M. Kowalski (Universitat Bonn), P. Nugent (LBL Berkeley), L. Wyrzykowski (Warsaw Observatory)
on 22 Dec 2013; 16:15 UT
Distributed as an Instant Email Notice Supernovae
Credential Certification: Sylvain Baumont (baumont@lpnhe.in2p3.fr)

Subjects: Optical, Supernovae

PESSTO, the Public ESO Spectroscopic Survey for Transient Objects (see Valenti et al., ATel #4037; http://www.pessto.org ), reports the following supernova classifications. Targets were supplied by the La Silla-Quest survey (see Hadjiyska et al., ATel #3812) and OGLE-IV (ATel #4495; Wyrzykowski et al. 2012). All observations were performed on the ESO New Technology Telescope at La Silla on 2013 Dec 21, 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 can be obtained from http://www.pessto.org (via WISeREP).

 
Name                 | RA (J2000)  | Dec (J2000) | Disc. Date | Disc. Source | Disc Mag  |  z   | Type  | Phase | Notes
OGLE-SN-2013-138 | 01:19:02.86 | -68:13:14.6 | 20131212 | OGLE | 18.6 | 0.115| IIn | ~max | (1) LSQ13dnd | 02:56:25.33 | -21:21:26.3 | 20131213 | LSQ | 19.9 | 0.115| Ia | +8 | LSQ13dlp | 04:48:11.60 | -24:53:17.5 | 20131210 | LSQ | 19.6 | 0.084| Ia | 0 | LSQ13doq | 11:34:35.07 | -24:05:14.4 | 20131217 | LSQ | 18.6 | 0.028| II | +6 | LSQ13dox | 11:28:26.44 | -07:39:16.4 | 20131218 | LSQ | 19.3 | 0.115| Ia | +8 | (2)

(1) blue continuum, narrow Ha and Hb.
(2) no galactic line is visible for a precise redshift estimate.