{
  "submitter": "EP Team at NAOC/CAS <ep_ta@bao.ac.cn>",
  "format": "text/plain",
  "subject": "The EP-WXT trigger 01709129287 is likely a flaring star",
  "bibcode": "2024GCN.38648....1L",
  "createdOn": 1734948979026,
  "body": "Q. C. Liu (THU), W. Chen, X. Mao, Z. X. Ling (NAO, CAS) report on behalf of the Einstein Probe team:\n\nThe EP-WXT trigger (ID 01709128948) on 2024-12-23 09:22:35 (UTC) is likely a stellar flare associated with a High Proper Motion Star TYC 5360-423-1. The estimated flux of the flare is around 2 x 10^-11 erg/s/cm^2 in 0.5-10.0 keV, corresponding to an X-ray luminosity of around 5 x 10^31erg/s.\n\nLaunched on January 9, 2024, EP is a space X-ray observatory to monitor the soft X-ray sky with onboard X-ray follow-up capability (Yuan et al. 2022, Handbook of X-ray and Gamma-ray Astrophysics).",
  "circularId": 38648,
  "submittedHow": "web"
}