EPTA second data release reports Bayes factor of 60 for an isotropic nanohertz GWB in the 10.3-year subset, with amplitude (2.5±0.7)×10^{-15} at 1 yr^{-1} when spectral index is fixed at 13/3.
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2 Pith papers cite this work. Polarity classification is still indexing.
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SHARP is positioned to deliver the first statistical census of ultra-compact dual AGN, bridging kpc-scale pairs to sub-pc binary MBHs that emit gravitational waves.
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The second data release from the European Pulsar Timing Array III. Search for gravitational wave signals
EPTA second data release reports Bayes factor of 60 for an isotropic nanohertz GWB in the 10.3-year subset, with amplitude (2.5±0.7)×10^{-15} at 1 yr^{-1} when spectral index is fixed at 13/3.
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A new era for Dual AGN science with SHARP
SHARP is positioned to deliver the first statistical census of ultra-compact dual AGN, bridging kpc-scale pairs to sub-pc binary MBHs that emit gravitational waves.