GCN Circular 14480

B. A. Zauderer, E. Berger, S. Chakraborti, and A. Soderberg (Harvard)
report on behalf of a larger collaboration:

"We observed the position of GRB 130427A (Maselli et al.; GCN 14448
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)
beginning 2013 Apr 27.99 (dt = 0.67 d) with the Very Large Array in its
D configuration (synthesized beam ~18'' x 11'').  At a mean frequency of 
~5.8 GHz, we detect a source with a flux of ~1 mJy +/- 20 uJy at a
position consistent with the optical afterglow (e.g. Elenin et al., 
Perley et al.; GCNs 14450
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, 14451
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). Followup observations are planned for 
this nearby z~0.34 GRB (Levan et al., Xu et al; GCNs 14455
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, 14478
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).

We thank the VLA observatory staff for their support of these observations."