GCN Circular 37304

WeiKang Zheng and Alexei V. Filippenko (UC Berkeley) report on

behalf of the KAIT GRB team:


The 0.76-m Katzman Automatic Imaging Telescope (KAIT), located at

Lick Observatory, responded to GRB 240825A (Gupta et al., GCN 37274
Not found
 
 
;

Fermi GBM team, GCN 37273
Not found
 
 
) starting at 05:36 UT, Aug. 26th, about

13.73 hours after the bust. Observations were performed in the clear

(roughly R) filter, and the exposure time was 60s per image, with a

total of 31 images were obtained. We clearly detected the optical

afterglow (Gupta et al., GCN 37274
Not found
 
 
; Jiang et al., GCN 37275
Not found
 
 
; Dutton

et al., GCN 37276
Not found
 
 
; Odeh et al., GCN 37277
Not found
 
 
, Zhang et al., GCN 37278
Not found
 
 
;

Li et al., GCN 37280
Not found
 
 
, Izzo et al., GCN 37287
Not found
 
 
; Lipunov et al., GCN

37289
Not found
 
 
; Leonini et al., GCN 37291
Not found
 
 
; Wu et al., GCN 37292
Not found
 
 
; Martin-Carrillo

et al., GCN 37293
Not found
 
 
; Brivio et al., GCN 37295
Not found
 
 
; Kuin et al., GCN 37296
Not found
 
 
;

Odeh et al., GCN 37299
Not found
 
 
; Le Floc’h et al., GCN 37300
Not found
 
 
; Guiffreda et al.,

GCN 37303
Not found
 
 
) in our coadd image, which we measured its brightness of

20.8 +/- 0.2 mag at a mid time of ~14.04 hours after the burst,

calibrated to the Pan-STARRS1 catalog.