GCN Circular 2993
D. A. Frail (NRAO) and A. M. Soderberg (Caltech) report on behalf of the Caltech-NRAO-Carnegie GRB Collaboration: "We have used the VLA to make observations of the XRT error circle (GCN #2984) for the Swift burst GRB050126 (GCN #2987). The observations were carried out on 2005 January 26.67 UT (4 hrs after the burst) and January 28.59 UT. At a frequency of 8.46 GHz no emission was detected above 135 microJy (4-5 sigma) within the 30-arcsec diameter error circle. At the position of the NIR afterglow candidate found by Berger and Kulkarni (GCN #2985) there is no emission in excess of 30-45 microJy. No further observations are planned."