Mass and spin measurements for the neutron star 4U1608−52 through the relativistic precession model
Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 486:4 (2019) 4485-4497
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.Study of the X-ray properties of the neutron star binary 4U 1728–34 from the soft-to-hard state
Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 484:3 (2019) 3004-3016
Accretion in strong field gravity with eXTP
Science China Physics, Mechanics & Astronomy Springer Nature 62:2 (2019) 29504
The long outburst of the black hole transient GRS 1716–249 observed in the X-ray and radio band
Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 482:2 (2019) 1587-1601