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GCN Circular 43266

Subject
EP251229a: NOT optical upper limits
Date
2025-12-30T10:31:06Z (5 hours ago)
From
Antonio Martin-Carrillo at UCD,Space Science Group <antonio.martin-carrillo@ucd.ie>
Via
Web form
A. Martin-Carrillo (UCD), J. Chacón (PUC), Z.P. Zhu, D. Xu (NAOC), G. Corcoran (UCD), F. E. Bauer (SSI and UTA), P.G. Jonker (Radboud) report on behalf of a larger collaboration:

We observed the field of the fast X-ray transient EP251229a (Wang et al., GCN 43253) using the Nordic Optical Telescope (NOT) equipped with the ALFOSC camera. Observations were obtained in the SDSS i and z bands consisting of 5x200 s exposures, starting on 2025-12-29 at 23:36:08 UTC (3.622 hours after the WXT trigger). 

No new source is detected within or at the border of the EP/FXT uncertainty region (Wang et al., GCN 43253). From the stacked images we obtain the following 3-sigma upper limits:


i > 24.0
z > 23.1

These upper limits are in AB magnitudes and were calibrated using nearby stars from the Pan-STARRS catalog and are not corrected for Galactic extinction.
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