{
  "eventType": [
    "X-ray Transient"
  ],
  "body": "Y. Wang (PMO, CAS; UCB), M. J. Liu (NAO, CAS), H. W. Peng (THU), H. W. Pan (NAO, CAS) on behalf of the Einstein Probe (EP) team:\n\nThe EP-WXT trigger 01709320790 at the time of 2026-09-29T14:56:13, is likely a stellar flare associated with BD-03 5579. The estimated flux of the flare is around 4.0x10^-11 erg/s/cm^2 in 0.5-4.0 keV, corresponding to an X-ray luminosity of around 1.3x10^31 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).\n",
  "subject": "The EP-WXT trigger 01709320790 is likely a flaring star",
  "circularId": 45785,
  "submittedHow": "web",
  "createdOn": 1790697063196,
  "submitter": "EP Team at NAOC/CAS <ep_ta@bao.ac.cn>",
  "format": "text/plain"
}