TITLE: GCN CIRCULAR NUMBER: 43495 SUBJECT: The EP-WXT trigger 01709251871 is likely a flaring star DATE: 26/01/22 01:53:51 GMT FROM: EP Team at NAOC/CAS <ep_ta@bao.ac.cn> R.D. Liang (NAOC), Z. X. Li, G. L. Huang, C. Wang (IHEP) and Y. Liu (NAOC) on behalf of the Einstein Probe (EP) team: The EP-WXT trigger 01709251871 at the time of 2026-01-22T00:00:14, is likely a stellar flare associated with [M81] I-308. The estimated flux of the flare is around 1x10^-10 erg/s/cm^2 in 0.5-4.0 keV, corresponding to an X-ray luminosity of around 8.5x10^31 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/43495. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0LW...