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GCN Circular 43875

Subject
EP260227a: Liverpool Telescope observations
Date
2026-02-28T10:29:52Z (12 days ago)
From
Rob Eyles-Ferris at U of Leicester <raje1@leicester.ac.uk>
Via
Web form

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

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) 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

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; 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)FilterAB magnitude
8.35g’>22.28 (3-sigma)
8.63i’21.12 +/- 0.08
8.92r’21.61 +/- 0.22
9.21z’20.74 +/- 0.11

Compared to the photometry tabulated by Fu et al. (GCN 43873

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) and Mandarakas et al. (GCN 43874), our observations suggest the source has not faded significantly between these three epochs.

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