{
  "subject": "GRB 241209A: EP-FXT follow-up observations",
  "format": "text/plain",
  "submitter": "Yu-Han Yang at University of Rome Tor Vergata <yyang@roma2.infn.it>",
  "bibcode": "2024GCN.38517....1T",
  "createdOn": 1733819786364,
  "circularId": 38517,
  "eventId": "GRB 241209A",
  "submittedHow": "web",
  "body": "E. Troja (U Rome), Y. L. Wang (NAO, CAS), Y. Wang (PMO, CAS), H. L. Peng (NNU), W. D. Zhang (NAO,CAS), Y. -H. Yang (U Rome), R. L. Becerra (U Rome) report on behalf of the Einstein Probe team:\n\nWe performed a follow-up observation of the short GRB 241209A detected by Fermi/GBM (GCN 38474) and Swift/BAT (GCN 38476) with the Follow-up X-ray Telescope (FXT) on board the Einstein Probe (EP) mission. The observation began at 2024-12-09T18:20:45 (UTC), about ~ 12.75 hours after the trigger, for a total exposure time of 4093 seconds.\n\nAt the position of the XRT counterpart (GCN 38486), we detect no new source. Assuming a photon index of 1.5 and a Galactic absorption of NH = 2E20 cm^-2, we derive an upper limit of ~3E-14 erg/cm2/s (0.5-10 keV; 90% confidence level). \n\nLaunched on January 9, 2024, EP is a space X-ray observatory to monitor the soft X-ray sky with X-ray follow-up capability (Yuan et al. 2022, Handbook of X-ray and Gamma-ray Astrophysics). EP is a mission of the Chinese Academy of Sciences in collaboration with ESA, MPE and CNES."
}