Detailed afterglow modelling and host galaxy properties of the dark GRB 111215A
Gamma-ray burst (GRB) 111215A was bright at X-ray and radio frequencies, but not detected in the optical or near-infrared (nIR) down to deep limits. We have observed the GRB afterglow with the Westerbork Synthesis Radio Telescope and Arcminute Microkelvin Imager at radio frequencies, with the Willia...
| Main Authors: | , , , , , , , , , , , , , , , |
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| Format: | Journal Article |
| Published: |
OXFORD UNIV PRESS
2015
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| Online Access: | http://hdl.handle.net/20.500.11937/20673 |