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- W2554258215 abstract "[Evidence] of polarized γ-ray emission (> 50 keV) from Gamma-Ray Bursts (GRBs) has been accumulated in recent years. Measurements have been reported with levels in the range of 30–80%, typically with limited statistical significance. No clear picture has yet emerged with regards to the polarization properties of GRBs. Taken at face value, the data suggest that most GRBs have a relatively large level of polarization (typically, > 50%), which may suggest synchrotron emission associated with an ordered magnetic field structure within the GRB jet. But these results are far from conclusive. Here, we review the observations that have been made, concentrating especially on the instrumental issues and the lessons that might be learned from these data." @default.
- W2554258215 created "2016-11-30" @default.
- W2554258215 creator A5087476135 @default.
- W2554258215 date "2017-02-01" @default.
- W2554258215 modified "2023-09-25" @default.
- W2554258215 title "High energy polarimetry of prompt GRB emission" @default.
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- W2554258215 doi "https://doi.org/10.1016/j.newar.2016.11.001" @default.
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