Large-amplitude late-time radio variability in GRB 151027B

Large-amplitude late-time radio variability in GRB 151027B

Context. Deriving physical parameters from gamma-ray burst (GRB) afterglow observations remains a challenge, even 20 years after the discovery of afterglows. The main reason for the lack of progress is that the peak of the synchrotron emission is in the sub-mm range, thus requiring radio observation...

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Bibliographic Details
Main Authors: Greiner, J., Bolmer, J., Wieringa, M., Van Der Horst, A., Petry, D., Schulze, S., Knust, F., De Bruyn, G., Krühler, T., Wiseman, P., Klose, S., Delvaux, C., Graham, J., Kann, D., Moin, A., Nicuesa-Guelbenzu, A., Schady, P., Schmidl, S., Schweyer, T., Tanga, M., Tingay, Steven, Van Eerten, H., Varela, K.
Format: Journal Article
Published: EDP Sciences 2018
Online Access:http://hdl.handle.net/20.500.11937/69739

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