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Spectroscopic classification of Gaia16atw and Gaia16aui with the SEDM (Spectra Energy Distribution Machine) on Palomar 60-inch (P60) telescope

ATel #9256; N. Blagorodnova, D. Neill, R. Walters (Caltech)
on 18 Jul 2016; 23:11 UT
Distributed as an Instant Email Notice Supernovae
Credential Certification: Nadejda Blagorodnova (nblago@ast.cam.ac.uk)

Subjects: Supernovae, Transient

The Caltech Time Domain Astronomy group reports the classification of Gaia16atw and Gaia16aui, discovered by the Gaia ESA survey. The observations were performed with the Spectral Energy Distribution Machine (SEDM)(http://www.astro.caltech.edu/sedm/, range 350-950nm, spectral resolution R~100) on Palomar 60-inch (P60) telescope.

 
Name                     | RA (J2000)  | Dec (J2000)   | redshift   |  Discovery (UT)     |  Discovery mag |  Type    | Phase      | Notes 
 
Gaia16atw                |  02:05:59.8 | +47:44:14.0  | 0.02       | 2016-07-08 08:07:52  | 18.40          |   IIn    |  +60 d     | (1) 
Gaia16aui                |  02:58:29.3 | +40:03:52.7  | 0.02       | 2016-07-12 08:12:27  | 18.33          |   Ia     |  +60 d     | (2) 
 

(1) Best fit template from SNID is SN1996L.
(2) Best fit template from SNID is the peculiar SN Ia - SN200cx.
Classifications were performed using SNID (Blondin and Tonry 2007, ApJ, 666, 1024).
We acknowledge ESA Gaia (http://cosmos.esa.int/gaia), and the DPAC Photometric Science Alerts Team (http://gsaweb.ast.cam.ac.uk/alerts) (Rixon et al, 2014, ATel #6593).