Super-massive black hole binaries are expected to produce a gravitational wave (GW) signal in the nano-Hertz frequency band which may be detected by pulsar timing arrays (PTAs) in the coming years. The signal is composed of both stochastic and individually resolvable components. Here we develop a generic Bayesian method for the analysis of resolvable sources based on the construction of ‘null-streams’ which cancel the part of the signal held in common for each pulsar (the Earth-term). For an array of N pulsars there are N − 2 independent null-streams that cancel the GW signal from a particular sky location. This method is applied to the localisation of quasi-circular binaries undergoing adiabatic inspiral. We carry out a systematic investig...
The couplings between supermassive black hole binaries (SMBHBs) and their environments within galact...
We have searched for continuous gravitational wave (CGW) signals produced by individually resolvable...
This manuscript focuses on the detection of low frequency (nanohertz) Gravitational Waves (GW) using...
Super-massive black hole binaries are expected to produce a gravitational wave (GW) signal in the na...
Pulsar Timing Arrays (PTAs) are sensitive to nanohertz gravitational waves (GWs), which affect the p...
We propose a novel methodology to select host galaxy candidates of future pulsar timing array (PTA) ...
Pulsar timing arrays (PTAs) might detect gravitational waves (GWs) from massive black hole (MBH) bin...
Pulsar timing arrays (PTAs) can be used to search for very low frequency (10−9–10−7 Hz) gravitationa...
Pulsar timing arrays (PTAs) are uniquely poised to detect the nanohertz-frequency gravitational wave...
Gravitational Waves (GWs) are tiny ripples in the fabric of spacetime predicted by Einstein\u27s the...
We consider the inverse problem in pulsar timing array (PTA) analysis, investigating what astrophysi...
The observation of massive black hole binaries (MBHBs) with Pulsar Timing Arrays (PTAs) is one of th...
This paper presents a technique to search for supermassive black hole binaries (MBHBs) in the Sloan ...
The sensitivity of Pulsar Timing Arrays to gravitational waves (GWs) depends on the noise present in...
Within the next several years, pulsar-timing array programs will likely usher in the next era of gra...
The couplings between supermassive black hole binaries (SMBHBs) and their environments within galact...
We have searched for continuous gravitational wave (CGW) signals produced by individually resolvable...
This manuscript focuses on the detection of low frequency (nanohertz) Gravitational Waves (GW) using...
Super-massive black hole binaries are expected to produce a gravitational wave (GW) signal in the na...
Pulsar Timing Arrays (PTAs) are sensitive to nanohertz gravitational waves (GWs), which affect the p...
We propose a novel methodology to select host galaxy candidates of future pulsar timing array (PTA) ...
Pulsar timing arrays (PTAs) might detect gravitational waves (GWs) from massive black hole (MBH) bin...
Pulsar timing arrays (PTAs) can be used to search for very low frequency (10−9–10−7 Hz) gravitationa...
Pulsar timing arrays (PTAs) are uniquely poised to detect the nanohertz-frequency gravitational wave...
Gravitational Waves (GWs) are tiny ripples in the fabric of spacetime predicted by Einstein\u27s the...
We consider the inverse problem in pulsar timing array (PTA) analysis, investigating what astrophysi...
The observation of massive black hole binaries (MBHBs) with Pulsar Timing Arrays (PTAs) is one of th...
This paper presents a technique to search for supermassive black hole binaries (MBHBs) in the Sloan ...
The sensitivity of Pulsar Timing Arrays to gravitational waves (GWs) depends on the noise present in...
Within the next several years, pulsar-timing array programs will likely usher in the next era of gra...
The couplings between supermassive black hole binaries (SMBHBs) and their environments within galact...
We have searched for continuous gravitational wave (CGW) signals produced by individually resolvable...
This manuscript focuses on the detection of low frequency (nanohertz) Gravitational Waves (GW) using...