GCN Circular 36367
Subject
LIGO/Virgo/KAGRA S240422ed: Host redshifts of AT2024hfq, AT2024hfu, and AT2024hmo from DBSP
Date
2024-05-02T00:00:10Z (2 years ago)
From
Tomas Ahumada Mena at Caltech <tahumada@caltech.edu>
Via
Web form
Tomas Ahumada (Caltech), Sam Rose (Caltech), Kaustav Das (Caltech), Mansi Kasliwal (Caltech), Igor Andreoni (UMD) report on behalf of the Zwicky Transient Facility (ZTF) collaboration:
We observed the candidates AT2024hfq, AT2024hfu, and AT2024hmo (GCN 36298, GCN 36303) with the Double Beam Spectrograph (DBSP) mounted on the Palomar 200-in telescope on 2024-05-01 (UTC), using a setup with a red grating of 316/7500, a blue grating of 600/400, a D55 dichroic, and a slitmask of 1.5". The data were reduced using a custom DBSP pipeline relying on Pypeit (Prochaska et al. 2019, Roberson et al. 2021).
We derived the redshifts from the H-alpha emission line of either the transient or the potential host. We conclude that these transients are unrelated to the event S240422ed, as all these are beyond 5-sigma of the median distance provided by the LVK skymap (GCN 36240).
AT name | redshift | notes
---------------------------
AT2024hfq