{
  "body": "Q. Y. Wu, Y. Liu (NAO, CAS), G. Gianfagna, A. L. Thakur (INAF-IAPS) on behalf of the Einstein Probe (EP) team:\n\nEP-FXT performed two follow-up observations of the IceCube-250706A (GCN 40994) (goldtrack) event. The first follow-up observation (obs1) started from 2025-07-06T13:56:24, about 40 minutes after the neutrino trigger, with an exposure time of 5.9 ks. The second one (obs2) started from 2025-07-06T21:01:14, about 8 hours after the trigger, with an exposure time of 4.1 ks. With the 1 deg x 1 deg FoV, EP-FXT covered most part of the 90% C.L. error region of the neutrino event. \n\nWithin the neutrino localization error region, only one source exhibited significant variability compared with historical fluxes or historical upper limits. The details are listed below:\nSource: EPF_J174217.4+392257\nRA (J2000): 265.5726\nDec (J2000): 39.3826\nPosition error in radius: 10 arcsec (90% C.L.) \nFlux in obs1: 1 x 10^-12 erg/s/cm2 (0.5-10 keV)\nFlux in obs2: not detected, with an upper limit around 5 x 10^-14 erg/s/cm2 (0.5-10 keV)\n \nA BY Dra variable star, ZTF J174217.39+392252.1, is 5 arcsec away from EPF_J174217.4+392257. Thus, the significant variability is likely due to the flare of this star with the X-ray luminosity of 6 x 10^30 erg/s.\n\nNo other source exhibited significant variability between the two observations. \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).",
  "version": 2,
  "createdOn": 1751968691721,
  "format": "text/plain",
  "bibcode": "2025GCN.41021....1W",
  "editedBy": "Judith Racusin at NASA/GSFC <judith.racusin@nasa.gov> on behalf of EP Team at NAOC/CAS <ep_ta@bao.ac.cn>",
  "editedOn": 1751986399972,
  "circularId": 41021,
  "eventId": "IceCube-250706A",
  "subject": "IceCube-250706A: EP-FXT follow-up observations",
  "submitter": "EP Team at NAOC/CAS <ep_ta@bao.ac.cn>",
  "submittedHow": "web"
}