A data analysis library for gravitational wave detection

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ID: 273182
2012
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Abstract
One of the main goals of Pulsar Timing Arrays (PTAs) is the direct detection of gravitational waves (GWs). A first detection will be a major leap for astronomy and substantial effort is currently going into timing as many pulsars as possible, with the highest possible accuracy. As part of the individual PTA projects, several groups are developing data analysis methods for the final stage of a gravitational-waves search pipeline: the analysis of the timing residuals. Here we report the progress of on-going work to develop, within a Bayesian framework, a comprehensive and user friendly analysis library to search for gravitational waves in PTA data.
Reference Key
vecchio2012proceedingsa Use this key to autocite in the manuscript while using SciMatic Manuscript Manager or Thesis Manager
Authors A. Lassus,R. van Haasteren,C. M. F. Mingarelli,K. J. Lee,A. Vecchio;A. Lassus;R. van Haasteren;C. M. F. Mingarelli;K. J. Lee;A. Vecchio;
Journal proceedings of the international astronomical union
Year 2012
DOI
10.1017/s1743921312024428
URL
https://sciprofiles.com/publication/view/4f507078af47b2d81be261115f30dda7
Keywords
methods: data analysis pulsars: general gravitational waves

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