Fig. 1
Radio contours (at 2×, 3×, 4×, and 5× the rms in each image) overplotted over the optical host images. The red circle is the GRB afterglow position with its uncertainty (see Table 3). The optical images are taken with VLT/FORS2/R (GRBs 000210, 050219, 090926B), VLT/ISAAC/J (GRB 030528), Gemini-N/MOS/R (GRB 020819B), HST/STIS (GRB 020127), HST/WFC3/F160W (GRBs 080319C, 080605, 081109, 090113, 100621A), and 2.2 m/GROND/r′ (GRB 110918A).
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