Fig. 16.

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Radio light curves of GRB 160131A at 11.4 GHz (top left), 13 GHz (top right), 18.8 GHz (bottom left), and 24.6 GHz (bottom right), obtained through a radio modelling (from radio to X-ray frequencies) for a FS model in ISM; we considered a jetted (edge-regime) emission with ISS effect, dust extinction and energy injection. Filled circles indicate detections, and upside-down triangles indicate 3σ upper limits; the red shaded regions represent the expected variability due to the ISS effect obtained through the prescription described in Misra et al. (2021).
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