A few well-timed VLA observations can distinguish relativistic, CSM-interacting, and off-axis GRB supernovae, but only if real light curves resemble the small template bank used in the simulations.
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An optimized radio follow-up strategy for stripped-envelope core-collapse supernovae
A few well-timed VLA observations can distinguish relativistic, CSM-interacting, and off-axis GRB supernovae, but only if real light curves resemble the small template bank used in the simulations.