GCN Circular 41267
Subject
GRB 250805A: Kilonova-Catcher optical upper limits
Event
Date
2025-08-07T15:27:58Z (4 months ago)
From
Damien Turpin at CEA-Saclay <dturpin-astro@hotmail.com>
Via
Web form
P. Jaquiery, R. Hellot (KNC), D. Turpin (CEA-Saclay/Irfu), C. Andrade(UMN), M. Pillas (ULiege), S. Antier (OCA/IJCLAB) on behalf of the GRANDMA/Kilonova-Catcher collaboration:
We observed the field of GRB 250805A (Ambrosi et al., GCN 41233) detected by Swift/BAT with the GRANDMA citizen science project Kilonova-catcher (KNC). Our observations were performed with a Celestron C14 telescope located at Beverly-Begg Observatory and operated by P. Jaquiery and the CDK17 telescope located at AITP San Pedro Chile Observatory operated by R. Hellot. Our observations started at T0+1.2hr.
In our stacked frames, subtracted from the Legacy Survey DR10 template image, we do not detect any optical counterpart inside the Swift/XRT position (Kennea et al., GCN 41234; Beardmore et al., GCN 41238) and at the position of the optical afterglow candidate reported by the VLT/X-shooter (Izzo et al., GCN 41241) and SVOM/VT (Li et al., GCN 41242) teams.
We report our follow-up results in the table below:
+---------------+-----------+------------+----------------------+-------------+
| Tmid-TGRB (hr)| Exp (s) | Filter | Magnitude | Instrument |
+===============+===========+============+======================+=============+
| 1.9 | 28 x 120s | sdssr (AB) | 18.3 (U.L., 5 sigma) | C14-BBO |
| 26.1 | 5 x 600s | sdssr (AB) | 19.5 (U.L., 5 sigma) | CDK17-AITP |
+---------------+-----------+------------+----------------------+-------------+
These upper limits are compatible with the magnitudes and upper limits reported by (Liu et al., GCN 41236