The Hubble parameter produces a frequency-independent angular enhancement in LISA timing residuals above 100 mHz, potentially enabling a percent-level H0 measurement without standard sirens.
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3 Pith papers cite this work, alongside 6 external citations. Polarity classification is still indexing.
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2026 3representative citing papers
Customized chromatic noise models for 67 pulsars detect non-dispersive delays in 21 cases, alter achromatic noise inferences in 19, and enable solar wind density estimates over 1.5 cycles.
Customized chromatic noise models applied to NANOGrav 15 yr data raise the Bayes factor for Hellings-Downs GWB correlations by a factor of ~8, lower the amplitude to 2.1e-15, and increase the spectral index to 3.5.
citing papers explorer
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Impact of $H_0$ on gravitational wave propagation: prospects for the LISA mission
The Hubble parameter produces a frequency-independent angular enhancement in LISA timing residuals above 100 mHz, potentially enabling a percent-level H0 measurement without standard sirens.
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The NANOGrav 15 yr Data Set: Customized Chromatic Noise Models
Customized chromatic noise models for 67 pulsars detect non-dispersive delays in 21 cases, alter achromatic noise inferences in 19, and enable solar wind density estimates over 1.5 cycles.
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The NANOGrav 15 yr Data Set: Impacts of Customized Chromatic Noise Models on Gravitational Wave Analyses
Customized chromatic noise models applied to NANOGrav 15 yr data raise the Bayes factor for Hellings-Downs GWB correlations by a factor of ~8, lower the amplitude to 2.1e-15, and increase the spectral index to 3.5.