Abstract. Gravitational wave astronomy will require the coordinated analysis of data from the global network of gravitational wave observatories. Questions of how to optimally con¯gure the global network naturally arise in this context. We propose a formalism to compare di®erent con¯gurations of the network, using both the coincident network analysis method and the coherent network analysis method, and construct a model to compute a ¯gure-of-merit based on the detection rate for a population of standard-candle binary inspirals. We ¯nd that this measure of network quality is very sensitive to the geographic location of component detectors under a coincident network analysis, but comparatively insensitive under a coherent network analysis
A network of gravitational wave detectors is called redundant if, given the direction to a source, t...
We derive a simple algebraic criterion to select the optimal detector network for a coherent wide pa...
At present several large-scale interferometric gravitational wave detectors including GEO, LIGO, TAM...
Gravitational wave astronomy will require the coordinated analysis of data from the global network o...
This paper develops a general framework for studying the effectiveness of networks of interferometri...
© 2019 IOP Publishing Ltd. Gravitational-wave astrophysics has the potential to be transformed by a ...
Abstract. This paper studies general properties of networks of interferometric gravitational wave de...
Spelling mistake corrected in one author\'s nameNetwork data analysis methods are the only way to pr...
Abstract. We consider the optimal site selection of future generations of gravitational wave detecto...
We compare two strategies of multidetector detection of compact binary inspiral signals, namely, the...
We derive a simple algebraic criterion to select the optimal detector network for a coherent wide pa...
We consider the optimal site selection of future generations of gravitational wave (GW) detectors. P...
The robust statistic proposed by Creighton and Allen et al. for detection in stationary non-Gaussia...
We formulate the data analysis problem for the detection of the Newtonian coalescing-binary signal b...
A network of gravitational wave detectors is called redundant if, given the direction to a source, t...
A network of gravitational wave detectors is called redundant if, given the direction to a source, t...
We derive a simple algebraic criterion to select the optimal detector network for a coherent wide pa...
At present several large-scale interferometric gravitational wave detectors including GEO, LIGO, TAM...
Gravitational wave astronomy will require the coordinated analysis of data from the global network o...
This paper develops a general framework for studying the effectiveness of networks of interferometri...
© 2019 IOP Publishing Ltd. Gravitational-wave astrophysics has the potential to be transformed by a ...
Abstract. This paper studies general properties of networks of interferometric gravitational wave de...
Spelling mistake corrected in one author\'s nameNetwork data analysis methods are the only way to pr...
Abstract. We consider the optimal site selection of future generations of gravitational wave detecto...
We compare two strategies of multidetector detection of compact binary inspiral signals, namely, the...
We derive a simple algebraic criterion to select the optimal detector network for a coherent wide pa...
We consider the optimal site selection of future generations of gravitational wave (GW) detectors. P...
The robust statistic proposed by Creighton and Allen et al. for detection in stationary non-Gaussia...
We formulate the data analysis problem for the detection of the Newtonian coalescing-binary signal b...
A network of gravitational wave detectors is called redundant if, given the direction to a source, t...
A network of gravitational wave detectors is called redundant if, given the direction to a source, t...
We derive a simple algebraic criterion to select the optimal detector network for a coherent wide pa...
At present several large-scale interferometric gravitational wave detectors including GEO, LIGO, TAM...