GCN Circular 37954

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

We observed the field of GRB 241029A (Fermi GBM team, GCN 37932
Not found
 
 
;
Schanne et al., GCN 37934
Not found
 
 
; Wang et al., GCN 37935
Not found
 
 
; Myers and Godwin,
GCN 37945
Not found
 
 
; Bernardini et al., GCN 37946
Not found
 
 
) with the 1-m telescope
of SAO RAS equipped with the CCD-photometer. We obtained 6 x 300 sec.
images in Rc band on October 29, 18:39:32--19:13:23 UT (16.6079 hours
after the burst).

The OT (Jiang et al., GCNs 37937
Not found
 
 
, 37940
Not found
 
 
; Lin et al., GCN 37939
Not found
 
 
;
Francile et al., GCN 37941
Not found
 
 
; Ackley et al., 37943; Odeh and Guessoum,
GCN 37944
Not found
 
 
; Adami et al., GCN 37948
Not found
 
 
; Fernandez et al., GCN 37950
Not found
 
 
)
is clearly detected in our stacked
frame with the brightness of R = 20.98 +/- 0.05 (R_lim = 23.0).
This preliminary photometry is based on nearby SDSS stars (magnitudes
converted with Lupton 2005 equations) and not corrected for the Galaxy
extinction.