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Observational manifestations of young neutron stars: Spin-powered pulsars
Michael Kramer
The largest number of known young neutron stars are observed as spin-powered pulsars. While the majority of those are detected at radio frequencies, an increasing number can be stu…
Giant pulses in Millisecond Pulsars
B. C. Joshi, M. Kramer, A. G. Lyne +2
Giant pulses (GPs), occasional individual pulses with an intensity 100 times the average intensity, have been detected in four pulsars todate. Their origin is not well understood,…
Long-Term Timing of 374 Pulsars
G. Hobbs, A. Lyne, M. Kramer
We have analysed the arrival times for 374 pulsars that have been observed for more than six years using the 76-m Lovell telescope at Jodrell Bank Observatory. Here we present a qu…
Pulsars with the SKA
Michael Kramer
As for other areas in modern astronomy, the SKA will revolutionize the field of pulsar astrophysics. Not only will new science be possible by the shear number of pulsars discovered…
Yet MORE PM Survey Discoveries....?
A. J. Faulkner, M. Kramer, G. Hobbs +9
The Parkes Multibeam (PM) survey has found nearly 50% of the >1400 known pulsars and detected 20% of the pulsars in binary systems (75% within the survey area), few of these are mi…
Polarisation Observations at Jodrell Bank Observatory
D. Athanasiadis, M. Kramer, I. H. Stairs +1
Some of the issues concerning polarisation calibration in the context of pulsar observations are outlined along with the existing calibration system in Jodrell Bank Observatory. Th…