PESSTO spectroscopic classification of optical transients
ATel #5250; C. Barbarino (INAF - Naples), A. De Cia, P. Vreeswijk, O. Yaron (Weizmann), M. T. Botticella (INAF - Naples), N. Elias-Rosa (ICE-IEEC/CSIC Barcelona), E. S. Walker (Yale), M. Nicholl (QUB), R. Scalzo (ANU), A. Gal-Yam (Weizmann), S. Benetti, A. Pastorello, (INAF - Padova), S. Valenti (LCOGT/UCSB), S. Taubenberger (MPA Garching), S. J. Smartt, K. Smith, D. Young, M. Fraser, C. Inserra (QUB), M. Sullivan (Uni. of Southampton), C. Knapic, M. Molinaro, R. Smareglia (Trieste), C. Baltay, N. Ellman, E. Hadjiyska, R. McKinnon, D. Rabinowitz (Yale), U. Feindt, M. Kowalski (Universitat Bonn), P. Nugent (LBL Berkeley), Lukasz Wyrzykowski (OGLE)
on 5 Aug 2013; 18:42 UT
Distributed as an Instant Email Notice Supernovae
Credential Certification: Ofer Yaron (ofer.yaron@weizmann.ac.il)
Subjects: Optical, Supernovae
Referred to by ATel #: 5251
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 the OGLE-IV Transient Search (see Wyrzykowski et al., ATEL #4495).
All observations were performed on the ESO New Technology Telescope at La Silla on 2013 August 05 (UT), using EFOSC2 and Grism 13 (3985-9315A, 18A resolution).
Classifications were done with SNID (Blondin & Tonry, 2007, ApJ, 666, 1024) and Superfit (Howell et al., 2005, ApJ, 634, 1190).
Classification spectra can be obtained from http://www.pessto.org via WISeREP (Yaron & Gal-Yam, 2012, PASP, 124, 668).
Name | RA (J2000) | Dec (J2000) | Disc. Date | Disc. Source | Disc Mag | z | Type | Phase | Notes
LSQ13baa | 16:27:48.83 | +19:38:37.3 | 2013-07-12 | LSQ | 19.6 | 0.082 | Gal | --- | (1)
LSQ13bbd | 22:39:04.84 | -10:17:24.3 | 2013-07-07 | LSQ | 20.4 | 0.07 | SN II | +20 | (2)
OGLE-2013-SN-040 | 00:53:49.35 | -63:49:24.3 | 2013-07-24 | OGLE | 19.3 | 0.09 | SN Ia | +5 | (3)
OGLE-2013-SN-041 | 01:36:18.01 | -69:34:12.6 | 2013-07-23 | OGLE | 19.4 | 0.10 | SN Ia | +3 | (3)
(1) Good match with a few starburst galaxy templates of Kinney et al. (1996)
(2) Balmer P-Cygni profiles. Good match with several type IIP SNe within ~5 days of the indicated phase.
(3) Good match with several normal type Ia SNe within ~5 days of the indicated phase.