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書目名稱Gravitational Wave Detection and Data Analysis for Pulsar Timing Arrays影響因子(影響力)




書目名稱Gravitational Wave Detection and Data Analysis for Pulsar Timing Arrays影響因子(影響力)學(xué)科排名




書目名稱Gravitational Wave Detection and Data Analysis for Pulsar Timing Arrays網(wǎng)絡(luò)公開(kāi)度




書目名稱Gravitational Wave Detection and Data Analysis for Pulsar Timing Arrays網(wǎng)絡(luò)公開(kāi)度學(xué)科排名




書目名稱Gravitational Wave Detection and Data Analysis for Pulsar Timing Arrays被引頻次




書目名稱Gravitational Wave Detection and Data Analysis for Pulsar Timing Arrays被引頻次學(xué)科排名




書目名稱Gravitational Wave Detection and Data Analysis for Pulsar Timing Arrays年度引用




書目名稱Gravitational Wave Detection and Data Analysis for Pulsar Timing Arrays年度引用學(xué)科排名




書目名稱Gravitational Wave Detection and Data Analysis for Pulsar Timing Arrays讀者反饋




書目名稱Gravitational Wave Detection and Data Analysis for Pulsar Timing Arrays讀者反饋學(xué)科排名

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簡(jiǎn)略

Narrative Means to Journalistic Endsnd time-dependent way) out to co-moving distances of ?billion light years. Modern predictions for black-hole merger rates imply marginal to modest chance of an individual jump detection by currently developed PTAs. The sensitivity is expected to be somewhat higher for futuristic PTA experiments with the Square Kilometre Array (SKA).

鴿子

https://doi.org/10.1007/978-3-319-22090-1ch is . times lower than the 95% confidence GWB limit obtained by the Parkes PTA in 2006. Our approach to the data analysis incorporates the multi-telescope nature of the European PTA and thus can serve as a useful template for future intercontinental PTA collaborations.

Proponent

,Was macht eine Erz?hlung zur Erz?hlung?,with its own frequency range. Every frequency range requires a different type of telescope to observe the radiation. Just as we cannot see radio signals with our eyes, we also need a different telescope to observe X-ray signals than to observe visible light.

使激動(dòng)

Gravitational-Wave Memory and Pulsar Timing Arrays,nd time-dependent way) out to co-moving distances of ?billion light years. Modern predictions for black-hole merger rates imply marginal to modest chance of an individual jump detection by currently developed PTAs. The sensitivity is expected to be somewhat higher for futuristic PTA experiments with the Square Kilometre Array (SKA).

使激動(dòng)

Placing Limits on the Stochastic Gravitational-Wave Background Using European Pulsar Timing Array Dch is . times lower than the 95% confidence GWB limit obtained by the Parkes PTA in 2006. Our approach to the data analysis incorporates the multi-telescope nature of the European PTA and thus can serve as a useful template for future intercontinental PTA collaborations.

我就不公正

Summary for Non-experts,with its own frequency range. Every frequency range requires a different type of telescope to observe the radiation. Just as we cannot see radio signals with our eyes, we also need a different telescope to observe X-ray signals than to observe visible light.

BUST

https://doi.org/10.1007/978-3-319-97825-3al waves. Several gravitational-wave observational programs, called Pulsar Timing Arrays (PTA), are being pursued around the world. Here we develop a Bayesian inference method for measuring the stochastic gravitational-wave background (GWB) from the PTA data. Our method has several strengths: (1) It

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