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GCN Circular 3543

XRF050509c: Radio Detection
2005-06-10T16:21:34Z (19 years ago)
Patrick B. Cameron at Caltech <>
P. B. Cameron and A. M. Soderberg (Caltech) report on behalf
of the Caltech-NRAO-Carnegie collaboration:

"We observed the field of XRF050509c (GCN 3402) with the
Very Large Array at 8.5 GHz on Jun 8.13 UT.  At the position of
the optical afterglow (GCN 3425) we detect a radio source
with flux density 310 +- 49 uJy.  Further observations are
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