Multi-wavelength observations of the GRB 080319B afterglow and the modeling constraints
Context: We present observations of the GRB 080319B afterglow at optical, mm, and radio frequencies between a few hours and 67 days after the burst. Aims: We attempt to understand the nature of this extraordinarily bright explosion based on the observed properties and its comparison with afterglow models. Methods: Our observations and other
Pandey, S. B. et al.
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2009