Spectroscopic Classifications of Optical Transients with the Lick Shane telescope
ATel #10593; D. A. Coulter, C. Rojas-Bravo, E. Xhakaj, Y.-C. Pan, C. D. Kilpatrick, R. J. Foley (UCSC)
on 23 Jul 2017; 22:59 UT
Credential Certification: Yen-Chen Pan (firstname.lastname@example.org)
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 PSST and ATLAS. All observations were made on 2017 July 22 UT. Classifications were performed with SNID (Blondin & Tonry, 2007, ApJ, 666, 1024).
Name | IAU Name | RA (J2000) | Dec (J2000) | z | Type | Phase | Notes
PS17dvb | AT2017fmv | 21:11:24.55 | +00:21:17.96 | 0.070 | Ia | +7 d |
PS17duz | AT2017fmu | 21:58:51.85 | -14:51:46.95 | 0.053 | Ia | +10 d |
PS17dvd | AT2017fne | 18:45:42.91 | +28:35:05.86 | 0.056 | Ia | +16 d |
ATLAS17ite | AT2017fnz | 22:29:42.86 | +11:48:16.70 | 0.081 | Ia | -2 d | (1)
PS17dvw | AT2017fod | 18:44:55.48 | +27:18:25.96 | 0.045 | 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 Si II 6355 velocity of -9,900 km/s.