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Gravitational wave astronomy with the SKA
G. H. Janssen, G. Hobbs, M. McLaughlin +12
On a time scale of years to decades, gravitational wave (GW) astronomy will become a reality. Low frequency (nanoHz) GWs are detectable through long-term timing observations of the…
The effect of small inter-pulsar distance variations in stochastic gravitational wave background searches with Pulsar Timing Arrays
Chiara M. F. Mingarelli, Trevor Sidery
One of the primary objectives for Pulsar Timing Arrays (PTAs) is to detect a stochastic background generated by the incoherent superposition of gravitational waves (GWs), in partic…
Mapping gravitational-wave backgrounds using methods from CMB analysis: Application to pulsar timing arrays
Jonathan R. Gair, Joseph D. Romano, Stephen Taylor +1
We describe an alternative approach to the analysis of gravitational-wave backgrounds, based on the formalism used to characterise the polarisation of the cosmic microwave backgrou…