GCN Circular 32757

T. Laskar (Utah), K. D. Alexander (Arizona), E. Ayache (Stockholm), E.
Berger (Harvard), R. Chornock (Berkeley), H. van Eerten (Bath), W. Fong
(Northwestern), R. Margutti (Berkeley), C.G. Mundell (Bath), and P. Schady
(Bath) report:

"We observed GRB 221009A (Dichiara et al. GCN 32632
Not found
 
 
) with the Karl G.
Jansky Very Large Array (VLA) beginning on 2022 October 12 23:08 UTC at
multiple frequencies (3.5 d after the burst). In preliminary analysis, we
detect the radio counterpart (Trushkin et al., ATEL 15671; Bright et al.,
GCN 32653
Not found
 
 
; Farah et al., GCN 32655
Not found
 
 
; Rhodes et al., GCN 32700
Not found
 
 
; Leung et al.,
GCN 32836
Not found
 
 
; Laskar et al., GCN 32740
Not found
 
 
) with a flux density of ~ 9.2 mJy at 11
GHz, and position:

RA (J2000) = 19:13:03.50
Dec (J2000) = 19:46:24.23

with a (statistical) uncertainty of 0.01" in each coordinate. This position
is consistent with the optical position (Dichiara et al., GCN 32632
Not found
 
 
;
Lipunov et al., GCN 32634
Not found
 
 
) and the radio position (Laskar et al., GCN
32740
Not found
 
 
). Further observations are planned.

We thank the VLA staff for scheduling and executing these observations"