{
  "createdOn": 1780629122316,
  "submittedHow": "web",
  "body": "R.-Z. Li (YNAO), X. Tian (GXU), C.-L. Guo and C.-C. Jin (NAOC) on behalf of the Einstein Probe (EP) team:\n\nThe EP-WXT trigger 01709266798 at the time of 2026-06-05T02:51:45, is likely a stellar flare associated with BD+33 2401 (High Proper Motion Star). The estimated flux of the flare is around 1.6 x 10^(-10) erg/s/cm^2 in 0.5-4.0 keV, corresponding to an X-ray luminosity of around 7.1 x 10^(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).",
  "subject": "The EP-WXT trigger 01709266798 is likely a flaring star",
  "submitter": "EP Team at NAOC/CAS <ep_ta@bao.ac.cn>",
  "format": "text/plain",
  "circularId": 44833
}