OzDES Spectroscopic Classification of DES13X3woy
ATel #5757; F. Yuan, M. Childress, R. Sharp (Australian National University); C. Lidman (Australian Astronomical Observatory); D. Parkinson (University of Queensland); J. Mould (Swinburne University of Technology); P. J. Brown, K. Krisciunas, N. Suntzeff (Texas A&M University); C. D'Andrea, R. Nichol, A. Papadopoulos (University of Portsmouth); M. Sullivan (University of Southampton); R. Maartens, M. Smith (University of the Western Cape); K. Barbary, J. P. Bernstein, R. Biswas, R. Gupta, E. Kovacs, S. Kuhlmann, H. Spinka (Argonne National Laboratory); E. Ahn, D. Finley, J. Frieman, J. Marriner, W. Wester (Fermilab); G. Aldering, J. S. Bloom, D. Goldstein, A. Kim, P. Nugent, S. Perlmutter, R. C. Thomas (Lawrence Berkeley National Laboratory); R. J. Foley (University of Illinois); S. Desai, K. Paech (Ludwig Maximilians University, Munich); R. C. Smith (NOAO/CTIO); M. Schubnell (University of Michigan); R. Kessler (University of Chicago); R. A. Covarrubias (University of Illinois / NCSA); R. Cane, J. A. Fischer, L. Gladney, M. March, M. Sako (University of Pennsylvania);
on 11 Jan 2014; 04:46 UT
Credential Certification: Fang Yuan (firstname.lastname@example.org)
Subjects: Optical, Supernovae
We report spectroscopic classification by OzDES of a supernova discovered
by the Dark Energy Survey (ATel #4668). The spectrum (370-885nm) was obtained
with the AAOmega Spectrograph (Saunders et al. 2004, SPIE, 5492, 389) and
the 2dF fibre positioner at the Anglo-Australian Telescope (AAT). Object
classification was performed using superfit (Howell and Wang, 2002, BAAS, 34, 1256), the
details of which are reported in the table below.
Name | RA (J2000) | Dec (J2000) | Discovery | Discovery | Spectrum | redshift | Type | Phase | Notes
| | | Date (UT) | r Mag | Date (UT) | | | |
DES13X3woy | 02 24 28.72 | -04 58 02.3 | 2013 Dec 01 | 22.2 | 2013 Dec 26 | 0.31 | I | - | Matches a SN Ibc at maximum light or a Ia two weeks after max.
The reduced spectrum has a number of artefacts that we hope to remove when we reprocess the data with a revised version of the