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experiments [ref] .","intent_p":0.88,"contests_p":null},{"arxiv_id":"2306.16213","title":"The NANOGrav 15-year Data Set: Evidence for a Gravitational-Wave Background","url":"/paper/2306.16213","section":"Implications for Gravitational Wave Observatories","sentence":"A NG string network with a tension as high as the best-fit value from Planck$+$BK18, $Gμ=7.8×10^-8$, would generate a Stochastic Gravitational Wave Background (SGWB) with an amplitude in the $n$Hz band that would exceed that of the signal recently reported by pulsar timing experiments [ref] .","intent_p":0.88,"contests_p":null},{"arxiv_id":"2306.16215","title":"Search for an isotropic gravitational-wave background with the Parkes Pulsar Timing Array","url":"/paper/2306.16215","section":"Implications for Gravitational Wave Observatories","sentence":"A NG string network with a tension as high as the best-fit value from Planck$+$BK18, $Gμ=7.8×10^-8$, would generate a Stochastic Gravitational Wave Background (SGWB) with an 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