Spectroscopic Classifications of Optical Transients with the Lick Shane telescope
ATel #10996; G. Dimitriadis, C. Rojas-Bravo, D. K. Reed, Y.-C. Pan, R. J. Foley (UCSC)
on 23 Nov 2017; 07:34 UT
Credential Certification: Yen-Chen Pan (ypan6@ucsc.edu)
Subjects: Optical, Supernovae
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 and ATLAS. All observations were made on 2017 Nov 22 UT. Classifications were performed with SNID (Blondin & Tonry, 2007, ApJ, 666, 1024).
Name | IAU Name | RA (J2000) | Dec (J2000) | z | Type | Phase | Notes
ATLAS17nan | AT2017hyf | 02:09:33.02 | +21:14:56.84 | 0.017 | Ib | +8 d |
ATLAS17ncr | AT2017hzc | 20:50:07.52 | +05:59:08.92 | 0.048 | Ia | +6 d | (1)
ATLAS17ndw | AT2017icw | 02:24:35.35 | -11:45:01.72 | 0.075 | Ia | +3 d | (2)
ATLAS17nek | AT2017iez | 01:33:13.24 | -17:31:31.71 | 0.046 | Ia | -1 d | (3)
ATLAS17nfs | AT2017ihl | 10:48:49.53 | -04:16:13.94 | 0.081 | Ia | +15 d |
ASASSN-17pl | AT2017ijw | 21:13:53.00 | +02:13:14.00 | 0.047 | Ia | +3 d | (4)
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 -9,600 km/s. We also detect Na D lines with EW = 1.5 A at the host-galaxy redshift and EW = 2.0 A at z = 0.
(2) We measure an Si II 6355 velocity of -10,700 km/s.
(3) We measure an Si II 6355 velocity of -11,500 km/s.
(4) We measure an Si II 6355 velocity of -9,800 km/s. We also detect Na D lines with EW = 2.3 A at the host-galaxy redshift and EW = 2.2 A at z = 0.