Spectroscopic Classifications of Optical Transients with the Lick Shane telescope
ATel #10620; E. Xhakaj, C. Rojas-Bravo, M. M. Foley, C. D. Kilpatrick, Y.-C. Pan, R. J. Foley (UCSC)
on 5 Aug 2017; 16:47 UT
Credential Certification: Yen-Chen Pan (firstname.lastname@example.org)
Subjects: Optical, Supernovae
Referred to by ATel #: 10668
We report the following classifications of optical transients from spectroscopic observations with the Kast spectrograph on the Shane telescope. Targets were supplied by ASAS-SN, ATLAS and Gaia. All observations were made on 2017 July 29 UT. Classifications were performed with SNID (Blondin & Tonry, 2007, ApJ, 666, 1024).
Name | IAU Name | RA (J2000) | Dec (J2000) | z | Type | Phase | Notes
Gaia17bvu | AT2017fqo | 01:53:01.51 | +12:42:46.04 | 0.015 | II | | (1)
ATLAS17izd | AT2017frj | 16:01:20.38 | +26:01:22.44 | 0.031 | Ia | -6 d | (2)
ATLAS17izf | AT2017frl | 16:37:48.60 | +11:47:30.67 | 0.070 | Ia | +1 d | (3)
ASASSN-17jz | AT2017fro | 17:19:55.90 | +41:40:49.33 | 0.165 | II | |
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 H alpha velocity of -5,600 km/s.
(2) We measure an Si II 6355 velocity of -13,900 km/s.
(3) We measure an Si II 6355 velocity of -10,200 km/s.