{
  "eventId": "EP261030a",
  "editedOn": 1793458714960,
  "body": "H.-H. Zhang, C.-Y. Dai (NJU), Y.-L. Wang (ICE, CSIC) and Y. Liu (NAOC) on behalf of the Einstein Probe (EP) team:\n\nWe report on the detection of a fast X-ray transient, designated EP261030a, identified in the downlinked data from the Wide-field X-ray Telescope (WXT) aboard the Einstein Probe (EP) mission. The WXT light curve of the transient began at about 2026-10-30T17:15:19 UTC and lasted for about 100 s. The WXT position of the source is R.A. = 23.663 deg, DEC = -11.691 deg (J2000) with an uncertainty of 3.2 arcmin in radius (90% C.L. statistical and systematic).\n\nThe 0.5-4 keV WXT spectrum can be fitted by an absorbed power-law model with a fixed Galactic column density of 2.4 x 10^20 cm^-2 and a photon index of 1.0 (-0.4,+0.4). The derived 0.5-4 keV unabsorbed flux is 3.6 (-0.9/+1.1) x 10^-10 erg/cm^2/s.\n\nA follow-up observation with the Follow-up X-ray Telescope (FXT) on board EP has been scheduled. Further information will be updated when the telemetry data is received.\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).",
  "submitter": "EP Team at NAOC/CAS <ep_ta@bao.ac.cn>",
  "format": "text/plain",
  "createdOn": 1793446196269,
  "subject": "EP261030a: Einstein Probe detection of a fast X-ray transient",
  "version": 2,
  "editedBy": "Judith Racusin at NASA/GSFC <judith.racusin@nasa.gov> on behalf of EP Team at NAOC/CAS <ep_ta@bao.ac.cn>",
  "eventType": [
    "X-ray Transient"
  ],
  "submittedHow": "web",
  "circularId": 46121
}