{
  "subject": "GRB 261029A: Fermi-LAT detection",
  "submittedHow": "web",
  "eventId": "GRB 261029A",
  "circularId": 46085,
  "submitter": "Rahul Gupta at NASA GSFC <rahul.gupta@nasa.gov>",
  "format": "text/markdown",
  "body": "F. Longo (Univ. and INFN, Trieste), T. Nymark (KTH), A. Holzmann Airasca (UniTrento and INFN Bari), and R. Gupta (NASA/GSFC) report on behalf of the Fermi-LAT collaboration:\n\nAt 01:27:03 UT on October 29th, 2026, Fermi-LAT detected high-energy emission from GRB 261029A, which was also detected by Fermi-GBM (trigger 814930028/261029060, GCN #46071) and SVOM (GCN #46072). Its optical counterpart was found by GOTO (GCN #46073) at a redshift of z = 3.27 using the NOT (GCN #46081).\n\nThe best LAT on-ground location is found to be\n\nRA, Dec = 9.69, 35.52 (J2000)\n\nwith an error radius of 0.57 deg (90 % containment, statistical error only).\n\nThis was 67 deg from the LAT boresight at the time of the trigger.\n\nThe data from the Fermi-LAT show a significant increase in the event rate that is spatially and temporally correlated with the trigger with high significance.\n\nThe photon flux above 100 MeV in the time interval 0 - 120 s after the GBM trigger is (9.4 ± 1.1)E-4 ph/cm2/s. The estimated photon index above 100 MeV is -2.80 ± 0.17. The highest energy photon has an energy of 2.5 GeV and occurs at 44 s after trigger time.\n\nThe Fermi-LAT point of contact for this burst is Riccardo Martinelli (riccardo.martinelli@phd.units.it).\n\nThe Fermi-LAT is a pair conversion telescope designed to cover the energy band from 20 MeV to greater than 300 GeV. It is the product of an international collaboration between NASA and DOE in the U.S. and many scientific institutions across France, Italy, Japan and Sweden.\n",
  "createdOn": 1793262047501,
  "eventType": [
    "GRB",
    "Gamma-ray Transient"
  ]
}