GCN Circular 36582

A. S. Moskvitin, O. I. Spiridonova and V. V. Vlasyuk (SAO RAS),
report on behalf of the GRB follow-up team.

We observed the field of the GRB 240529A (Eyles-Ferris et al.
GCN 36556
Not found
 
 
; Osborne et al. GCN 36557
Not found
 
 
; Joshi et al. GCN 36560
Not found
 
 
;
Dichiara et al. GCN 36564
Not found
 
 
; Markwardt et al. GCN 36566
Not found
 
 
; Tan et al.
GCN 36578
Not found
 
 
) with the SAO RAS 1m telescope Zeiss-1000 equipped
with CCD-photometer. We obtained 4 x 300 sec frames in Rc band
on May 30, 23:35:04--23:56:50 UT (t_mid - T0 = 1.8663 days).

The OT (Kumar et al. GCN 36559
Not found
 
 
; Fu et al. GCN 36561
Not found
 
 
; Shilling et al.
GCN 36562
Not found
 
 
; Perez-Garcia et al. GCN 36563
Not found
 
 
; Dutton et al. GCN 36568
Not found
 
 
;
Mo et al. GCN 36569
Not found
 
 
; Odeh et al. GCN 36573
Not found
 
 
; de Ugarte Postigo et al.
GCN 36574
Not found
 
 
; Adami et al. GCN 36575
Not found
 
 
; Mohan et al. GCN 36576
Not found
 
 
;
Vinko et al., GCN 36577
Not found
 
 
; Lim et al. GCN 36579
Not found
 
 
) is clearly detected
in the stacked frame with the brightness of R = 20.02 +/- 0.10.

The magnitudes were calibrated using R2 magnitudes of nearby USNO-B1.0
stars.