Spectroscopic Classification of Optical Transients with the Lick Shane telescope
ATel #16877; K. C. Patra, K. Taggart, R. J. Foley (UCSC)
on 25 Oct 2024; 16:50 UT
Distributed as an Instant Email Notice Supernovae
Credential Certification: Kirsty Taggart (k.taggart@ucsc.edu)
Subjects: Optical, Supernovae
We report the following classifications of optical transients from spectroscopic observations with the Kast spectrograph on the Shane telescope. The targets were supplied by the Young Supernova Experiment, ATLAS, GOTO and ZTF. All observations were made on 2024 Oct 24 UT. Classifications were performed with SNID (Blondin & Tonry, 2007, ApJ, 666, 1024).
Name | IAU Name | RA (J2000) | Dec (J2000) | z | Type | Phase|
GOTO24gxy | 2024xol | 03:24:03.51 | -15:43:02.23 | 0.08 | Ia | +3 |
PS24jlq | 2024xqf | 22:45:08.10 | +24:27:39.30 | 0.061 | Ia | +4 |
ZTF24abmhrjk | 2024yfk | 02:51:55.47 | -04:57:33.48 | 0.09 | Ia | +2 |
ATLAS24por | 2024yyu | 22:59:39.40 | +20:08:11.55 | 0.024 | II | |
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.
