{
  "editedBy": "Judith Racusin at NASA/GSFC <judith.racusin@nasa.gov> on behalf of Zipei Zhu at NAOC <zpzhu@nao.cas.cn>",
  "bibcode": "2026GCN.44140....1Z",
  "subject": "EP-WXT trigger 01709259209: TRT optical counterpart detection",
  "submittedHow": "web",
  "body": "Z.P. Zhu (NAOC), S. Tinyanont, K. Noysena, K. Chanchaiworawit, S. Tinyanont (NARIT), J. An, X. Liu, S.Q. Jiang, L.B. He, N.C. Sun, W.X. Li, D. Xu (NAOC), S.Y. Fu (HUST) report on behalf of a large collaboration:\n\nWe observed the field of EP260329a detected by the Einstein Probe (EP) (Trigger ID: 01709259209 ), using the 0.7-m telescope of the Thai Robotic Telescope network (TRT), located at Sierra Remote Observatories in California.\n\nThe uncatalogued source is located at:\n\nR.A. (J2000) = 12:05:14.95 \nDec.( J2000) = +4:21:05.8\n\nwith an uncertainty of ~ 0.8 arcsec.\n\nThe optical counterpart is clearly detected in the stacked image with the measured brightness of R = 18.4 +/- 0.1 at a mid-time of 10:47:20 UTC on 2026-03-29, consistant with the optical candidate  reported by LCO (Li et al., GCN 44139), calibrated using nearby stars from the Pan-STARRS catalog and are not corrected for Galactic extinction.",
  "circularId": 44140,
  "submitter": "Zipei Zhu at NAOC <zpzhu@nao.cas.cn>",
  "createdOn": 1774783958028,
  "editedOn": 1774882600102,
  "format": "text/plain",
  "version": 2
}