Einstein Probe detects fast X-ray transient EP260210a with no optical counterpart

AI Summary

EP260210a, a short-lived X-ray transient detected by Einstein Probe's WXT, showed an average unabsorbed 0.5-4 keV flux of 1.5 × 10^(-10) erg/s/cm^2. Follow-up observations by various ground-based telescopes set stringent upper limits on potential optical counterparts without detecting any new sources.

Measurements

Event ID01709257873
SourceEinstein Probe WXT
Alert typeGRB
Significancehigh
Trigger time (UTC)Tue, 10 Feb 2026 10:23:01 GMT
Right ascension (J2000)169.84°
Declination (J2000)45.408°
Position error radius0.05121313°
Image SNR7.6
GCN notices1
GCN circulars8

Notices (1)

Einstein Probe WXT — GRB · Tue, 10 Feb 2026 10:23:01 GMT

GCN Circulars (8)

GCN-43773 — EP260210a · Tue, 17 Feb 2026 15:04:00 GMT
The IKI-GRB-FuN team reports non-detection of a new optical source in the error circle of the fast X-ray transient EP260210a using the AZT-33IK 1.5m telescope at Mondy observatory. The only catalogued source within the error circle, a galaxy at (J2000) 11:19:19.81 +45:23:43.8, was detected and its R-band magnitudes were measured as 20.29±0.05 and 20.31±0.06 on Feb 10 and Feb 14, respectively.

GCN-43697 — EP260210a · Wed, 11 Feb 2026 15:54:23 GMT
An astronomical alert was issued regarding the observation of transient object EP260210a by the MASTER-Tunka robotic telescope in Russia. The team pointed the telescope to the errorbox 1 day after the notice time and obtained upper limits on the object's brightness in clear filter C, ranging from 18.1 to 20.9 mag. The observations are ongoing.

GCN-43696 — EP260210a · Wed, 11 Feb 2026 14:20:01 GMT
The Einstein Probe (EP) mission detected a fast X-ray transient, EP260210a, with its Wide-field X-ray Telescope (WXT). The event started on February 10, 2026, and lasted for approximately 220 seconds. The derived average unabsorbed 0.5-4 keV flux was 1.5 (-0.3/+0.4) × 10^(-10) erg/s/cm^2. The Follow-up X-ray Telescope (FXT) on board EP observed the source a few minutes later and detected an uncatalogued source with an average unabsorbed 0.5-10 keV flux of 6.4 (-1.1/+1.1) × 10^(-12) erg/s/cm^2 and a photon index of 2.7 (-0.1/+0.1). The FXT observation had an effective exposure time of around 5 ks.

GCN-43692 — EP260210a · Wed, 11 Feb 2026 08:35:06 GMT
Astronomical alert: EP260210a: Optical upper limits with Kinder observations

GCN-43687 — EP260210a · Tue, 10 Feb 2026 17:33:25 GMT
The SVOM/VT team performed a Target of Opportunity observation of EP260210a, a transient phenomenon detected by the Einstein Probe. No uncatalogued sources were detected within the error box of EP-FXT, and the 3 sigma limit magnitudes in the VT_B and VT_R channels were found to be greater than 23.2 mag and 22.9 mag, respectively. These limits are consistent with earlier upper limits from SVOM/C-GFT and COLIBRÍ.

GCN-43684 — EP260210a · Tue, 10 Feb 2026 14:47:40 GMT
A team of international researchers using the COLIBRÍ telescope at the Observatorio Astronómico Nacional in Mexico conducted follow-up observations of the transient event EP260210a. They did not detect any new source at the position of the event and reported 5-sigma upper limits for the r and z bands: r > 23.59 and z > 22.15.

GCN-43683 — EP260210a · Tue, 10 Feb 2026 13:35:22 GMT
The SVOM/C-GFT team reported no credible candidate detection within the error box of EP260210a in their g, r, and i-band follow-up imaging using the Chinese Ground Follow-up Telescope (C-GFT). The team obtained upper limits for magnitudes in each band: i-band (20.02), g-band (20.15), and r-band (20.23). These limits were calibrated against the UCAC4 catalogue.

GCN-43681 — EP260210a · Tue, 10 Feb 2026 12:13:39 GMT
The Einstein Probe mission, a space X-ray observatory, has detected an X-ray transient designated EP260210a using its Wide-field X-ray Telescope (WXT). The transient, located at R.A. = 169.840°, DEC = 45.408° (J2000), triggered the WXT on February 10, 2026. An uncatalogued X-ray source was later identified within the error circle using the Follow-up X-ray Telescope (FXT). This discovery marks a significant finding in X-ray astronomy.

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AI summary generated Sat, 14 Mar 2026 08:34:40 GMT.