Spectroscopic Classification of ASAS-SN Transients
ATel #6293; J. L. Prieto (Universidad Diego Portales), B. J. Shappee, T. W.-S. Holoien, K. Z. Stanek, A. B. Davis, C. S. Kochanek, J. Jencson, U. Basu, J. F. Beacom (Ohio State), D. Bersier (LJMU), D. Szczygiel, G. Pojmanski (Warsaw University Observatory), J. Brimacombe (Coral Towers Observatory)
on 6 Jul 2014; 10:36 UT
Credential Certification: Jose L. Prieto (jose.prietok@mail.udp.cl)
Subjects: Optical, Cataclysmic Variable, Supernovae, Transient
We report optical spectroscopic observations of ASAS-SN transients (ATel #6252, #6269, #6277, #6283) obtained on UT July 7 with IMACS (range 3600-9600 Angstroms) mounted on the 6.5-m Magellan Baade Telescope. We used SNID (Blondin & Tonry, 2007, ApJ, 666, 1024) to aid with the type and phase of the SN spectra.
Name | Disc. ATel | Spec. Type | Phase | Best SN template |
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ASASSN-14cu | 6252 | Ia | +19d | SN 2001bg |
ASASSN-14dd | 6269 | Ibn | +6d | SN 2006jc |
ASASSN-14di | 6277 | II | +16d | SN 1999em |
ASASSN-14dl | 6283 | II | +1d | SN 2004et |
ASASSN-14dn | | CV | | |
ASASSN-14do | | CV | | |
We thank LCOGT and its staff for their continued support of ASAS-SN. For more information about the ASAS-SN project, see the ASAS-SN Homepage and the list of all ASAS-SN transients.
