{
  "submitter": "u6074340@umail.utah.edu",
  "subject": "GRB 260924A: VLA detection",
  "submittedHow": "web",
  "createdOn": 1790617389325,
  "body": "A. Gulati (University of Utah), T. Laskar (University of Utah), K. D. Alexander (University of Arizona), D. Eappachen (University of Utah), C. Christy (University of Arizona), N. Franz (University of Arizona)\n\nWe observed GRB 260924A (Fermi GBM, GCN 45712; D’Elia et al., GCN 45713) with the Karl G. Jansky Very Large Array (VLA) at multiple frequencies beginning on 2026 Sep 26 at 14:36 UT (2.6 days after the burst). \n\nIn preliminary analysis, we detect a radio counterpart at 15 GHz with a flux density of ~0.6 mJy at the position:\n\nRA (J2000) = 08:55:03.106 +/- 0.001” \nDec (J2000) = +12.02.35.24 +/- 0.03” \n\nThis is consistent with the X-ray position (Evans et al., GCN 45715) and optical position (Izzo et al., GCN 45718; Klingler et al., GCN 45735). Further observations are planned. \n\nWe thank the VLA staff for scheduling and executing these observations.\n",
  "eventType": [
    "GRB",
    "Radio Transient"
  ],
  "eventId": "GRB 260924A",
  "circularId": 45776,
  "format": "text/plain"
}