TITLE: GCN CIRCULAR NUMBER: 45426 SUBJECT: The EP-WXT trigger 01709287395 is likely a flaring star DATE: 26/08/23 01:46:42 GMT FROM: EP Team at NAOC/CAS <ep_ta@bao.ac.cn> Y.Q. Zhao(USTC,PRIC), B. Zhang, J. P. Feng (USTC), H. Sun (NAO,CAS) on behalf of the Einstein Probe (EP) team: The EP-WXT trigger 01709287395 at the time of 2026-08-22T20:31:42, is likely a stellar flare associated with HD197192. The source is located at ~ 40pc and has a history X-ray detection. The estimated flux of the flare is around 3.65e-11 erg/s/cm^2 in 0.5-4.0 keV, corresponding to an X-ray luminosity of around 7.08e30 erg/s. Launched 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). View this GCN Circular online at https://gcn.nasa.gov/circulars/45426. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0LW...