{
  "body": "R. Ricci, M. Yadav, E. Troja (U Rome) report:\n\nWe observed the short-duration GRB 260114A detected by Fermi-GBM (Fermi team GCN 43395), Swift/BAT (Eyles-Ferris et al. GCN 43396), GECAM-B (Ren et al., GCN 43402) and SVOM/GBM (SVOM/GRM team, GCN 43404) with Very Large Array in C-band at the centre frequency of 6 GHz with a bandwidth of 4 GHz on Jan 15th 2025, 15.5 hours after the burst. \n\nAfter reducing the data using the CASA version v6.6.1 with standard procedures no source was detected inside the Swift/XRT error circle (Eyles-Ferris et al., GCN 43396) down to a 3-sigma flux density upper limit of about 30 microJy/beam. \n \nWe thank the VLA staff for promptly executing the observations. \n\n",
  "circularId": 43411,
  "submitter": "Roberto Ricci at INAF-IRA <ricci@ira.inaf.it>",
  "createdOn": 1768475489655,
  "subject": "GRB 260114A: 6 GHz VLA observations",
  "bibcode": "2026GCN.43411....1R",
  "eventId": "GRB 260114A",
  "submittedHow": "web",
  "format": "text/plain"
}