GCN Circular 36318

A. de Ugarte Postigo (CNRS/OCA & LAM), M. Bremer (IRAM), C. C. Thoene (ASU-CAS), J. F. Agui Fernandez (CAHA), S. Antier (OCA), S. Basa (LAM), M. Michalowski (AOI-AMU), D. A. Perley (LJMU), J.-G. Ducoin (CPPM) report:

We observed the field of GRB 240414A (Caputo et al. GCN 36083
Not found
 
 
; Myers et al. GCN 36120
Not found
 
 
; Cheung et al. GCN 36147
Not found
 
 
) with the NOEMA interferometer, located at the Plateau de Bure (France). The observation, performed on the 23rd April, was tuned with sidebands at 74 and 90 GHz.

When combining all the data, we obtain a weak, 3-sigma detection at the position of the afterglow (Schneider et al. GCN 36084
Not found
 
 
; Adami et al. GCN 36085
Not found
 
 
; de Ugarte Postigo GCN 36087
Not found
 
 
; Dutton et al. 36097; Turpin et al. GCN 36101
Not found
 
 
; Osborne et al. GCN 36102
Not found
 
 
; Dichiara et al. GCN 36104
Not found
 
 
; Pankov et al. GCN 36113
Not found
 
 
; Siegel et al. GCN 36115
Not found
 
 
; de Ugarte Postigo et al. GCN 36117
Not found
 
 
; Wang et al. GCN 36131
Not found
 
 
; Rossi et al. GCN 36228
Not found
 
 
; Rhodes et al. GCN 36229
Not found
 
 
; Giarratana et al. GCN 36231
Not found
 
 
) with a flux density of ~55 uJy.

Based on observations carried out under project number W23DI with the IRAM NOEMA Interferometer. IRAM is supported by INSU/CNRS (France), MPG (Germany) and IGN (Spain).