{
  "circularId": 41844,
  "bibcode": "2025GCN.41844....1W",
  "submitter": "EP Team at NAOC/CAS <ep_ta@bao.ac.cn>",
  "body": "B.T. Wang (YNAO, CAS), S. Q . Jiang, W. D. Zhang (NAO, CAS) on behalf of the Einstein Probe (EP) team:\n\nThe EP-WXT trigger 01709241037 at the time of 2025-09-16T23:34:38 (UTC), is likely a stellar flare associated with UPM J0113-5939. The estimated flux of the flare is around 6e-11 erg/s/cm^2 in 0.5-4.0 keV, corresponding to an X-ray luminosity of around 1.3e31 erg/s.\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).",
  "submittedHow": "web",
  "subject": "The EP-WXT trigger 01709241037 is likely a flaring star",
  "createdOn": 1758075425674,
  "format": "text/plain"
}