GCN Circular 43441
Subject
GRB 260117A: SVOM/VT optical candidate
Event
Date
2026-01-18T08:09:33Z (7 days ago)
From
Huali Li at at NAOC, SVOM <lhl@nao.cas.cn>
Via
Web form
H. L. Li, C. Wu, Y. N. Ma, Y. L. Qiu, Z. H. Yao, L.P. Xin, X. H. Han, J. Wang, Y. Xu, P. P. Zhang, W. J. Xie, Y. J. Xiao, H. B. Cai, L. Lan, J. R. Xu, J. S. Deng, J. Y. Wei (NAOC), J. T. Palmerio, D. Adrien(CEA/Irfu) report on behalf of the SVOM/VT team.
SVOM/VT performed ToO observation for the long faint burst GRB 260117A triggered by SVOM/ECLAIRs (sb26011705, Palmerio et al., GCN 43437). The observation started at 2026-01-17T22:14:53 UTC, i.e., 2.398 hours post trigger in the VT_B (400nm-650nm) and VT_R (650nm-1000nm) channels simultaneously.
An uncatalogued source was detected only in VT_R stacked images within the error box of EP/FXT and source 1 from Swift-XRT (Salvaggio et al., GCN 43439; Evans et al., GCN 43438), compared to the Legacy survey catalog. It is also located in the error box of ECLAIRs (Palmerio et al., GCN 43437). The position is at R.A., Dec. = 188.138564, 43.912747 degrees, equivalent to:
R.A. (J2000) = 12:32:33.25
Dec. (J2000) = +43:54:45.89
with an uncertainty of 0.5 arcsec.
The measurements in AB magnitudes are given below:
Mid_time Band Exposure Time Magnitude (AB)
4.36 hour VT_R 68*70 sec 22.98+/-0.25
4.36 hour VT_B 73*70 sec >23.8
Our photometry was not corrected for Galactic extinction.
The Space Variable Objects Monitor (SVOM) is a China-France joint mission led by the Chinese National Space Administration (CNSA, China), National Center for Space Studies (CNES, France) and the Chinese Academy of Sciences (CAS, China), which is dedicated to observing gamma-ray bursts and other transient phenomena in the energetic universe. VT was jointly developed by Xi'an Institute of Optics and Precision Mechanics (XIOPM), CAS and National astronomical observatories (NAOC), CAS.