A detailed radio study of the energetic, nearby, and puzzling GRB 171010A
Monthly Notices of the Royal Astronomical Society Oxford University Press 486:2 (2019) 2721-2729
Abstract:
We present the results of an intensive multi-epoch radio frequency campaign on the energetic and nearby GRB 171010A with the Karl G. Janksy Very Large Array and Arcminute Microkelvin Imager Large Array. We began observing GRB 171010A a day after its initial detection, and were able to monitor the temporal and spectral evolution of the source over the following weeks. The spectra and their evolution are compared to the canonical theories for broad-band GRB afterglows, with which we find a general agreement. There are, however, a number of features that are challenging to explain with a simple forward shock model, and we discuss possible reasons for these discrepancies. This includes the consideration of the existence of a reverse shock component, potential microphysical parameter evolution, and the effect of scintillation.Low-frequency Faraday rotation measures towards pulsars using LOFAR: probing the 3D Galactic halo magnetic field
Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 484:3 (2019) 3646-3664
What do astronomers want from the STFC?
Astronomy and Geophysics Oxford University Press 60:2 (2019) 2.13-2.17
Abstract:
Stephen Serjeant and the STFC's Astronomy Advisory Panel summarize community responses to its consultation on research priorities, undertaken in November 2018.Identifying transient and variable sources in radio images
Astronomy and Computing Elsevier 27 (2019) 111-129
A detailed radio study of the energetic, nearby and puzzling GRB 171010A
(2019)