Spectroscopic classification of AT2019ugu and AT2019ugv
ATel #13286; Chien-Hsiu Lee (NSF's OIR Lab), Monika Soraisam (UIUC), Gautham Narayan (UIUC), Thomas Matheson (NSF's OIR Lab), Abhijit Saha (NSF's OIR Lab), Arizona-NOAO Temporal Analysis and Response to Events System (ANTARES) team, Thomas G. Brink, Kishore C. Patra, Thomas de Jaeger, WeiKang Zheng, Benjamin E. Stahl, Alexei V. Filippenko (UC Berkeley), Daniel Muthukrishna (University of Cambridge)
on 12 Nov 2019; 16:11 UT
Credential Certification: Chien-Hsiu Lee (lee@noao.edu)
Subjects: Optical, Supernovae, Transient
We report the classification of AT2019ugu and AT2019ugv from spectroscopic observations with the Kast spectrograph on the 3 m Shane telescope at Lick Observatory. The optical spectra were obtained on 2019 November 6 UT. Targets were flagged and supplied by ANTARES (antares.noao.edu) and our customized filter as promising stellar explosion events. Classification was performed with DASH (Muthukrishna et al. 2019, arXiv:1903.02557). The light curve of AT2019ugu and AT2019ugv can be found at: https://antares.noao.edu/alerts/data/321743884 and https://antares.noao.edu/alerts/data/308491448 , respectively.
Name | IAU Name | RA (J2000) | Dec (J2000) | MJD | z. | Type | Phase | Notes
ZTF19acmdpyr | AT2019ugu | 18:05:33.94 | +45:15:16.36 | 58793.07 | 0.045 | Ia | near max. | (1)
ZTF19acbwmqd | AT2019ugv | 00:01:21.63 | +34:36:27.88 | 58793.12 | 0.11 | Ia | near max. | (1)
Note: (1) AT2019ugu and AT2019ugv were both reported to TNS by ZTF as candidate supernovae.
