AstroNote 2024-94

Primary tabs

DRAFT
2024-04-07 19:26:57
Type: Object/s-Discovery/Classification
AT2024fkm - Spectroscopic classification as a type IIb supernova from Keck/LRIS
Authors: Viraj Karambelkar (Caltech), Robert Stein (Caltech), Shreya Anand (Caltech), Tomas Ahumada (Caltech), Mansi Kasliwal (Caltech), Igor Andreoni (UMD), Michael Lundquist (Keck), Jesper Sollerman (OKC), Anna Ho (Cornell), Michael Coughlin (U. Minnesota), Sean Brennan (OKC), Varun Bhalerao (IIT Bombay), G.C. Anupama (IIA), Fabio Bresolin (U. Hawaii)
Source Group: ZTF
Keywords: Supernova
Abstract:
We report the spectroscopic classification of the fast-fading transient AT2024fkm as a type IIb supernova.

We observed the fast-fading transient AT2024fkm / ZTF24aaifosg / ATLAS 24evb (Astronotes 2024-92, 2024-93) with the Low Resolution Imaging Spectrometer (LRIS, Oke et al. 95) on the Keck I telescope, with observations beginning at UTC 2024-04-07 15:31:17. We took two 1200s blue exposures, and four 600s red exposures. These data were reduced with lpipe (Perley et al. 2019). 

The spectrum shows broad features of hydrogen with P-cygni line profiles at z=0.041, consistent with the redshift of the host galaxy UGC 08802. Cross-matches to supernova templates using SNID (Blondin & Tonry 2007), show that the spectrum closely resembles the type IIb SN 1993J at a phase of 2 days before peak (see attached plot).

Show current TNS values
CatalogNameReported RAReported DECReported Obj-TypeReported RedshiftHost NameHost RedshiftRemarksTNS RATNS DECTNS Obj-TypeTNS Redshift
TNS2024fkm13:53:08.541+35:43:13.78SN IIb0.04113:53:08.564+35:43:14.38SN IIb0.04113