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GCN Circular 41499

Subject
GRB 250806A: Gemini observations of host galaxy candidate
Date
2025-08-22T16:12:48Z (2 days ago)
From
gsriniv2@umd.edu
Via
Web form
C. Sevilla (Cornell), G. Srinivasaragavan (UMD), D. A. Perley (LJMU), A. Y. Q. Ho (Cornell), A. Bochenek (LJMU) report:

We observed the candidate host galaxy of GRB 250806A (Xie et al., GCN 41243, Malesani et al. GCN 41279) beginning UTC 2025-08-13 13:14:40 with the Gemini Multi-Object Spectrograph on Gemini North under program GN-2025B-Q-125 (PI: Srinivasaragavan).  We use a 1 arcsecond slit, the R400 grating, and the GG455 filter.  We obtained four exposures of 450 seconds each, two at a central wavelength of 520 nm and two at 525 nm.

We obtain a redshift of 0.367 from galactic Hβ, [O II], and [O III] emission lines. At this redshift, using the 4 - 120 keV flux from Bouchet et al. (GCN 41287) and observed burst time of 20 seconds, we estimate the burst has an isotropic equivalent energy of ~ 8e49 erg.  

We thank the Gemini Contact Scientists and the Gemini Helpdesk for their assistance in observing and data reduction.

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