GCN Circular 45947
Subject
EP261006a : MeerKAT radio observations.
Event
Date
2026-10-14T10:18:12Z (7 days ago)
From
stephane.corbel@cea.fr
Via
Web form
S. Corbel, N. Grollimund (Université Paris Cité & CEA Saclay), Chichuan Jin (National Astronomical Observatories), Alexis Coleiro, Zheyu Lin (Université Paris Cité) report :
We observed the field of the fast X-ray transient EP261006a (Lao et al. GCN 45826) with the MeerKAT radio telescope at two frequencies: L-band [central frequency: 1.284 GHz / Bandwidth: 856 MHz] and S-band [central frequency: 3.062 GHz / Bandwidth: 875 MHz]
Data were calibrated and imaged using standard procedures. J1939-6342 was used for flux density and bandpass calibration whereas J0108+0134 (L-band) /J0121+0422 (S-band) were used for complex gain calibration.
Observations were conducted on two days:
2026-10-09 (16 min/band),
L-band
Start: 2026-10-09 20:41:01 UTC
Central MJD 61322.87 (t-t0 = 3.12 days)
S-band
Start: 2026-10-09 19:42:28 UTC
Central MJD 61322.83 (t-t0 = 3.08 days)
and
2026-10-11 (16 min/band)
L-band
Start: 2026-10-11 20:02:31 UTC
Central MJD 61324.84 (t-t0 = 5.10 days)
S-band
Start: 2026-10-11 18:48:18 UTC
Central MJD 61324.79 (t-t0 = 5.05 days)
By combining both observations per band, no radio source is detected at the candidate optical counterpart (Eyles-Ferris et al. GCN 45831; Wu et al. GCN 45852; Bochenek & Perley GCN 45853; Chen et al. GCN 45854) down to a preliminary 3-sigma upper limit of 39 uJy/beam (L-band) and 27 uJy/beam (S-band). This is in agreement with the concomitant non detection reported by the VLA at 10 GHz around the same period (Yadav et al. GCN 45921