TITLE: GCN CIRCULAR NUMBER: 37228 SUBJECT: EP240801a: Keck/LRIS spectroscopic redshift confirmation DATE: 24/08/22 08:10:26 GMT FROM: Weikang Zheng at UC Berkeley WeiKang Zheng, Thomas G. Brink, Alexei V. Filippenko (UCB), Rebecca Davies and Adam Deller (Swinburne), report on behalf of the KAIT GRB team: Following the detection of EP240801a (Zhou et al., GCN 36997), we observed its GRB optical counterpart (Fu et al., GCN 36998; Li et al., GCN 36999; Zheng et al., GCN 37000; Aryan et al., GCN 37002; An et al., GCN 37004; Pérez-Fournon et al., GCN 37007; Malesani et al., GCN 37008; Zhu et al., GCN 37010; Moskvitin & Spiridonova, GCN 37012; Quirola-Vásquez et al., GCN 37013; Moretti et al., GCN 37014; Turpin et al., GCN 37015; Pankov et al., GCN 37016; Moskvitin & Spiridonova, GCN 37017; Ruocco et al., GCN 37024; Pankov et al., GCN 37040; Moskvitin et al., GCN 37049; Pankov et al., GCN 37146) with the Low Resolution Imaging Spectrometer (LRIS, Oke et al. 1995) at the Keck I Observatory (ToO program U232, PI A. V. Filippenko). Observations started at 2024-08-02 09:36 (~1.02 days after the burst), and consisted of 3 x 950 s exposures with the 600/4000 grism and 400/8500 grating. The spectrum shows a well-detected continuum. We detect narrow absorption lines consistent with Mg II 2796, 2803 Ang doublet as well as Fe II 2600 Ang, confirming the redshift of z = 1.673 reported by Quirola-Vásquez et al. (GCN 37013) from GTC. We thank Josh Walawender and Matthew Wahl from the Keck team for their support during this Target of Opportunity trigger. The data presented herein were obtained at the W. M. Keck Observatory, which is operated as a scientific partnership among the California Institute of Technology, the University of California, and the National Aeronautics and Space Administration. The Observatory was made possible by the generous financial support of the W. M. Keck Foundation. The authors wish to recognize and acknowledge the very significant cultural role and reverence that the summit of Maunakea has always had within the indigenous Hawaiian community. We are most fortunate to have the opportunity to conduct observations from this mountain.