Spectroscopic Classification of AT2023uru with SOAR/Goodman
ATel #16325; K. W. Davis, R. J. Foley (UCSC)
on 6 Nov 2023; 22:31 UT
Distributed as an Instant Email Notice Supernovae
Credential Certification: Ryan Foley (foley@ucsc.edu)
Subjects: Optical, Supernovae
We report the following the classification of AT2023uru from spectroscopic observations with the Goodman spectrograph on the SOAR telescope using the AEON queue, made on 2023 Oct 27 UT. The target was supplied by CRTS and identified using the target management platform YSE-PZ (Coulter et al., 2023, PASP, 135, 4501). The classification was performed with SNID (Blondin & Tonry, 2007, ApJ, 666, 1024).
Name | IAU Name | RA (J2000) | Dec (J2000) | z | Type | Phase | Notes
| AT2023uru | 00:23:16.008 | +24:57:17.36 | 0.060 | II |post-peak| (1)
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 a H-alpha absorption velocity of -14,500 km/s.
We thank the SOAR observatory staff for executing this observation.
