GCN Circular 43875
R. A. J. Eyles-Ferris and N. R. Tanvir (Leicester) report on behalf of a larger collaboration:
We observed the field of EP260227a (Wang et al., GCN 43869) with the 2m Liverpool Telescope on La Palma using the IO:O instrument. We obtained 6x150s exposures in each of the SDSS g’ r’ i’ z’ filters starting at 2026-02-28 04:25:03 UT, approximately 8.21 hours after the X-ray detection.
We detect the optical counterpart (Eyles-Ferris et al., GCN 43867; Li et al., GCN 43868; Fu et al., GCN 43873; Mandarakas et al., GCN 43874) in the r’, i’ and z’ bands. We measure the following magnitudes calibrated to Pan-STARRS and not corrected for Galactic extinction.
| t_mid (hours) | Filter | AB magnitude |
|---|---|---|
| 8.35 | g’ | >22.28 (3-sigma) |
| 8.63 | i’ | 21.12 +/- 0.08 |
| 8.92 | r’ | 21.61 +/- 0.22 |
| 9.21 | z’ | 20.74 +/- 0.11 |
Compared to the photometry tabulated by Fu et al. (GCN 43873) and Mandarakas et al. (GCN 43874), our observations suggest the source has not faded significantly between these three epochs.