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Understanding pulsar magnetospheres with the SKA
A. Karastergiou, S. Johnston, N. Andersson +14
The SKA will discover tens of thousands of pulsars and provide unprecedented data quality on these, as well as the currently known population, due to its unrivalled sensitivity. He…
Understanding the Neutron Star Population with the SKA
Thomas M. Tauris, Victoria M. Kaspi, Rene P. Breton +9
Since their discovery in the late 1960's the population of known neutron stars (NSs) has grown to ~2500. The last five decades of observations have yielded many surprises and demon…
The unusual glitch recoveries of the high magnetic field pulsar J11196127
D. Antonopoulou, P. Weltevrede, C. M. Espinoza +4
Providing a link between magnetars and radio pulsars, high magnetic field neutron stars are ideal targets to investigate how bursting/magnetospheric activity and braking torque var…
Understanding the spin-down rate changes of PSR B0919+06
B. B. P. Perera, B. W. Stappers, P. Weltevrede +2
We study the spin-down properties of PSR B0919+06 based on almost 30 years of radio observations. We confirm that the time derivative of the rotational frequency is modula…
Investigating the magnetic inclination angle distribution of -ray-loud radio pulsars
S. C. Rookyard, P. Weltevrede, S. Johnston
Several studies have shown the distribution of pulsars' magnetic inclination angles to be skewed towards low values compared with the distribution expected if the rotation and magn…
Constraints on viewing geometries from radio observations of -ray-loud pulsars using a novel method
S. C. Rookyard, P. Weltevrede, S. Johnston
We present radio intensity and polarisation profiles of 28 -ray-detected pulsars with the aim of putting constraints on their viewing geometries using data from the Parkes teles…