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GCN Circular 42710

Subject
GRB 251111A: Mondy optical upper limit
Date
2025-11-17T08:05:29Z (5 days ago)
From
Alina Volnova at IKI RAS <alinusss@gmail.com>
Via
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A. Volnova (IKI), E. Klunko (ISTP), A. Pozanenko (IKI) report on behalf of IKI-GRB-FuN:

We observed the field of the GRB 251111A (Cheng et al., GCN 42637) with the AZT-33IK 1.5m telescope of the Sayan Solar Observatory (Mondy) in the R-filter starting Nov., 11, 2025, UT 16:26:22, and taking several frames with 120 s exposures. In the stacked frame we do not detect the optical counterpart (López-Cámara et al., GCN 42638; Wu et al., GCNs 42639, 42641; Ma et al., GCN 42647). Preliminary photometry is the following:

Date        UT start  t-T0       Exp.    Filter  OT     Err.  UL     
                     (mid,days)  (n*s)                       (3sigma)
2025-11-11  16:26:22  0.48686    25*120  R       n/d    n/d   22.1

The photometry is based on several nearby SDSS stars (R-magnitudes Lupton's transformation) and is not corrected for the Galactic extinction, all magnitudes are in Vega system.
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