GCN Circular 37017

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

We observed the field of the fast X-ray transient EP240801a
(Zhou et al., GCN 36997
Not found
 
 
) with the SAO RAS 1-meter telescope Zeiss-1000
equipped with the CCD-photometer. We obtained 9 x 300 sec frames
in Rc band on 2024-08-02T20:14:00 -- 2024-08-02T22:09:01 (UTC),
t_mid - T0 = 1.5038 days.

The OT (Fu et al., GCN 36998
Not found
 
 
; Li et al., GCN 36999
Not found
 
 
; Zheng et al.,
GCN 37000
Not found
 
 
; Aryan et al., GCN 37002
Not found
 
 
; An et al., GCN 37004
Not found
 
 
;
Perez-Fournon et al., GCN 37007
Not found
 
 
; Malesani et al., GCN 37008
Not found
 
 
;
Zhu et al., GCN 37010
Not found
 
 
; Quirola-Vasquez et al., GCN 37013
Not found
 
 
;
Moretti et al., GCN 37014
Not found
 
 
; Turpin et al., GCN 37015
Not found
 
 
; Pankov et al.,
GCN 37016
Not found
 
 
) is clearly detected in the stacked frame
with the brightness of R = 22.17 +/- 0.15, calibrated against nearby
Pan-STARRS stars and not corrected for Galactic extinction.