Placing limits on the stochastic gravitational‐wave background using European Pulsar Timing Array data

Placing limits on the stochastic gravitational‐wave background using European Pulsar Timing Array data

Source :

• Monthly Notices of the Royal Astronomical Society [ 0035-8711 ] ; 2011-07-11.

English descriptors

• KwdEn :
  • Algorithm, Archival arecibo data, Backer, Bayesian, Bayesian algorithm, Bayesian analysis, Best estimates, Binary, Characteristic strain, Characteristic strain spectrum, Correlation matrices, Cosmic strings, Damour vilenkin, Data analysis, Data sets, Deterministic processes, Different data sets, Different epta observatories, Different observatories, Different radio telescopes, Dispersion measure, Efac, Efac parameter, Efac value, Effelsberg, Effelsberg toas, Epta, Epta data, Epta data sets, Epta telescopes, Equad parameter, Equad parameters, Error bars, Functional form, General relativity, Gravitational waves, Haasteren, Hobbs, Hobbs edwards, Hole binaries, Jaffe backer, Jenet, Large number, Limit calculation, Lovell telescope, Marginalized, Marginalized posteriors, Millisecond pulsars, Mnras, Model parameter, Model parameters, Monthly notices, More pulsars, Multitelescope nature, Nancay radio telescope, Noise amplitude, Noise component, Noise parameters, Observatory, Other pulsars, Other timing model parameters, Parameter, Parameter space, Posterior distribution, Previous section, Probability distribution, Pulsar, Pulsar timing, Pulsar timing observations, Pulse freq, Quantum grav, Radio telescope, Radiometre noise, Residual, Respective volume, Same pulsar, Several telescopes, Single pulsar, Spectral index, Stochastic, Stochastic background, Stochastic processes, Strict periodicity, String tension, Supermassive, Systematic contributions, Telescope, Tempo2, Timing, Timing model, Timing model parameters, Timing noise, Timing residuals, Timing solution, Timing solutions, Toas, Upper limit, Upper limits, Vhlml, Vilenkin, White noise, Wsrt, Wyithe loeb.
• Teeft :
  • Algorithm, Archival arecibo data, Backer, Bayesian, Bayesian algorithm, Bayesian analysis, Best estimates, Binary, Characteristic strain, Characteristic strain spectrum, Correlation matrices, Cosmic strings, Damour vilenkin, Data analysis, Data sets, Deterministic processes, Different data sets, Different epta observatories, Different observatories, Different radio telescopes, Dispersion measure, Efac, Efac parameter, Efac value, Effelsberg, Effelsberg toas, Epta, Epta data, Epta data sets, Epta telescopes, Equad parameter, Equad parameters, Error bars, Functional form, General relativity, Gravitational waves, Haasteren, Hobbs, Hobbs edwards, Hole binaries, Jaffe backer, Jenet, Large number, Limit calculation, Lovell telescope, Marginalized, Marginalized posteriors, Millisecond pulsars, Mnras, Model parameter, Model parameters, Monthly notices, More pulsars, Multitelescope nature, Nancay radio telescope, Noise amplitude, Noise component, Noise parameters, Observatory, Other pulsars, Other timing model parameters, Parameter, Parameter space, Posterior distribution, Previous section, Probability distribution, Pulsar, Pulsar timing, Pulsar timing observations, Pulse freq, Quantum grav, Radio telescope, Radiometre noise, Residual, Respective volume, Same pulsar, Several telescopes, Single pulsar, Spectral index, Stochastic, Stochastic background, Stochastic processes, Strict periodicity, String tension, Supermassive, Systematic contributions, Telescope, Tempo2, Timing, Timing model, Timing model parameters, Timing noise, Timing residuals, Timing solution, Timing solutions, Toas, Upper limit, Upper limits, Vhlml, Vilenkin, White noise, Wsrt, Wyithe loeb.

Abstract

• https://api.istex.fr/document/844CF7F1713E2E0C5BA7491E0AF3024404E6072A/fulltext/pdf

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