{
  "circularId": 46132,
  "submitter": "EP Team at NAOC/CAS <ep_ta@bao.ac.cn>",
  "subject": "The EP-WXT trigger 01709322206 is likely a flaring star",
  "eventType": [
    "X-ray Transient"
  ],
  "body": "Z.M. Wang (BNU), Q.Y. Wu (NAOC), H. Sun (NAOC) on behalf of the Einstein Probe (EP) team:\n\nThe EP-WXT trigger 01709322206 at the time of 2026-11-02 23:26:00, is likely a stellar flare associated with HG 7-33. The estimated flux of the flare is around 1.2e-10 erg/s/cm^2 in 0.5-4.0 keV, corresponding to an X-ray luminosity of around 2.8e31 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",
  "createdOn": 1793665526550,
  "format": "text/plain"
}