Spectroscopic Classifications of Optical Transients with the Lick Shane 3-m telescope
ATel #11622; G. Dimitriadis, R. J. Foley (UCSC)
on 9 May 2018; 00:38 UT
Credential Certification: Georgios Dimitriadis (gdimitri@ucsc.edu)
Subjects: Optical, Supernovae
We report the following classifications of optical transients from spectroscopic observations with the Kast spectrograph on the Shane 3-m telescope. Targets were supplied by ATLAS, ASAS-SN, and the KEGS K2 SN search. All observations were obtained on 2018 May 08 UT. Classifications were performed with SNID (Blondin & Tonry, 2007, ApJ, 666, 1024).
Name | IAU Name | RA (J2000) | Dec (J2000) | z | Type | Phase | Notes
ATLAS18nut | AT2018bfd | 14:29:00.52 | +17:19:30.63 | 0.052 | Ia | +2d | (1)
ASASSN-18jn | AT2018bfh | 10:22:41.19 | +15:56:20.11 | 0.044 | Ia | +5d | (2)
ASASSN-18jp | AT2018bfr | 11:04:47.50 | -15:37:59.20 | 0.072 | Ia | -1d | (3)
C17-0118 | AT2018bft | 13:53:19.15 | -04:51:31.87 | 0.075 | Ia | -3d | (4,5)
Notes:
When the redshift is given to 2 decimal places, it is derived from the SN spectrum. Otherwise, the redshift is determined from the host galaxy.
(1) We measure an Si II 6355 velocity of -11,300 km/s.
(2) We measure an Si II 6355 velocity of -9,800 km/s.
(2) We measure an Si II 6355 velocity of -10,800 km/s.
(4) We measure an Si II 6355 velocity of -12,700 km/s.
(5) This is in a K2 Campaign 17 galaxy and should be observed by K2.