PESSTO spectroscopic classification of optical transients
ATel #5842; F. Taddia, M. Ergon (Stockholm), G. Leloudas (Stockholm/DARK), J. Sollerman (Stockholm), C. Inserra (QUB), R. Scalzo (Australian National University), S. Benetti, A. Pastorello (Padova), S. Smartt, K. Smith, D. Young (QUB), M. Sullivan (Southampton), S. Taubenberger (MPA), S. Valenti (LCOGT), M. Fraser (IoA), O. Yaron, A. Gal-Yam, I. Manulis (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), D. Wright, R. Kotak, (QUB), W. Burgett, K. Chambers, M. Huber, R. P. Kudritzki, E. Magnier, J. Morgan, C. Stubbs, W. Sweeney, J. Tonry, C. Waters (IfA, Univ. Hawaii), P. Draper, N. Metcalfe (Univ. of Durham), A. Rest (STScI)
on 1 Feb 2014; 16:01 UT
Distributed as an Instant Email Notice Supernovae
Credential Certification: Francesco Taddia (ftadd@astro.su.se)
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), Pan-STARRS (see Valenti et al., ATel #2668) and
the Catalina Real-time Transient Survey (http://crts.caltech.edu). All observations were performed
on the ESO New Technology Telescope at La Silla on 2014 February 01 UT, 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
CSS140128-045040+200126 | 04:50:39.52 | +20:01:26.1 | 20140128 | CRTS | 19.0 | 0 | ? | ? | (1)
PS1-14ip | 08:08:12.86 | -08:31:13.6 | 20140120 | PS1 | 17.6 | 0 | star | - |
LSQ14mc | 09:02:13.45 | +17:03:37.1 | 20140129 | LSQ | 19.2 | 0.057 | Ia | pre-max |
LSQ14ko | 12:23:34.50 | -22:21:12.6 | 20140128 | LSQ | 20.0 | 0.07 | Ia | pre-max |
LSQ14jn | 13:02:18.01 | -16:21:59.9 | 20140125 | LSQ | 19.5 | 0.096 | Ia | max |
PS1-14gj | 13:19:32.99 | +16:38:40.8 | 20140117 | PS1 | 18.3 | 0.023 | Ia | +80d |
(1) The spectrum exhibits narrow Balmer lines in emission at z=0.