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GCN Circular 41934

Subject
GRB 250916A: SAO RAS Zeiss-1000 optical observations
Date
2025-09-22T09:39:39Z (8 hours ago)
From
Alexander Moskvitin at SAO RAS <mosk@sao.ru>
Via
Web form
A. Moskvitin, O. Spiridonova (SAO), N. Pankov (HSE), A. Pozanenko 
(IKI), A. Ghosh, S. Razzaque (CAPP, University of Johannesburg), 
Tao An and Yuanqi Liu (Shanghai Astronomical Observatory) 
report on behalf of GRB follow-up collaboration and IKI-GRB-FuN.

We observed the field of the GRB 250916A (Fermi GBM team, GCN 41839; 
Arya et al., GCN 41843; Cheung et al., GCN 41855; Osborne et al., 
GCN 41862; Waratkar and Grefenstette, GCN 41871; Godwin and Meegan, 
GCN 41876) with the 1-m SAO RAS telescope Zeiss-1000 equipped 
with the CCD-photometer. We obtained 9 x 300 sec. images Rc band 
on September 21, 23:36:57 -- September 22, 00:47:22 UT 
(t_mid - T0 = 5.44639 days).

The optical transient (Belkin et al., GCN 41847; Mohan et al., 
GCN 41858; Moskvitin et al., GCN 41859; Burkhonov et al., GCN 41860;
de Ugarte Postigo et al., GCN 41863; Moskvitin et al., GCN 41870;
Zheng and Filippenko, GCN 41873; Pankov et al., GCN 41892; 
Hall et al., GCN 41921) is clearly detected in the stacked frame 
with the brightness of R = 22.6 +/- 0.1.

Date        UT start  t-T0     Exp.  Filter  OT     Err. UL (3sigma)
                      (mid, d) (s)       
2025.09.21  23:36:57  5.44639  9 x 300 Rc  22.6 +/- 0.1 23.3
                      
Preliminary photometry is based on the nearby objects from PanSTARRS 
(magnitudes converted with Lupton 2005 equations) 
and has not corrected for the Galactic extinction.
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