ePESSTO spectroscopic classification of optical transients
ATel #12588; L. Tartaglia (Stockholm Univ.), V. Brinnel (HU Berlin), A. S. Carracedo, C. Barbarino, J. Sollerman (Stockholm Univ.), R. Cartier (CTIO), J. Lyman (Warwick), C. Inserra (Cardiff), E. Kankare (Turku), K. Maguire, S. J. Smartt, D. R. Young, K. W. Smith, O. McBrien (QUB), O. Yaron, I. Manulis (Weizmann), J. Tonry, L. Denneau., A. Heinze, H. Weiland (IfA, Univ. of Hawaii), B. Stalder (LSST), A. Rest (STScI), D. E. Wright (Univ. of Minnesota)
on 17 Mar 2019; 17:51 UT
Credential Certification: Leonardo Tartaglia (leonardo.tartaglia@astro.su.se)
Subjects: Optical, Supernovae, Transient
Referred to by ATel #: 12604
ePESSTO, the extended 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) and the Zwicky Transient Facility (https://www.ztf.caltech.edu/; Kulkarni et al. 2018, ATel #11266) data stream processed through the Lasair broker (http://lasair.roe.ac.uk/). All observations were performed on the ESO New Technology Telescope at La Silla on 2019-03-16, 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
ATLAS19dyw | AT2019bus | 14 29 25.70 | +16 40 55.88 | 20190315 | ATLAS | 19.76 | 0.085 | Ia-91T | -8d | (1)
ZTF19aajwogx | | 12 02 50.90 | -16 39 54.00 | 20190210 | ZTF | 20.20 | ? | young II ? | ? | (2)
ZTF19aalwegb | | 05 23 51.39 | +08 54 59.10 | 20190305 | ZTF | 19.86 | 0.072 | Ia-norm | +1d | (1)
(1) Redshift is given by SNID.
(2) Blue continuum (T~10000 K) with shallow features.