The Stochastic Siren: Astrophysical Gravitational-Wave Background Measurements of the Hubble Constant
astro-ph.CO, gr-qc
Submitted: 2025-03-03
Updated: 2026-08-31
Terminology
Sources
- The Hubble Tension and Early Dark Energy
- A Comprehensive Measurement of the Local Value of the Hubble Constant with 1 km/s/Mpc Uncertainty from the Hubble Space Telescope and the SH0ES Team
- The local and distant Universe: stellar ages and $H_0$
- A Measurement of the CMB Temperature Power Spectrum and Constraints on Cosmology from the SPT-3G 2018 TT/TE/EE Data Set
- DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations
- Determining the Hubble constant from gravitational wave observations of merging compact binaries
- First measurement of the Hubble constant from a dark standard siren using the Dark Energy Survey galaxies and the LIGO/Virgo binary-black-hole merger GW170814
- Gravitational Radiation, Inspiraling Binaries, and Cosmology
- Striking a Chord with Spectral Sirens: multiple features in the compact binary population correlate with $H_0$
- GW150914: Implications for the stochastic gravitational wave background from binary black holes
- The population of merging compact binaries inferred using gravitational waves through GWTC-3
- Detecting a stochastic background of gravitational radiation: Signal processing strategies and sensitivities
- Detection methods for stochastic gravitational-wave backgrounds: a unified treatment
- Distance measures in cosmology
- Mining Gravitational-wave Catalogs To Understand Binary Stellar Evolution: A New Hierarchical Bayesian Framework
- Extracting distribution parameters from multiple uncertain observations with selection biases
- Inferring the properties of a population of compact binaries in presence of selection effects
- ICAROGW: A python package for inference of astrophysical population properties of noisy, heterogeneous and incomplete observations
- Detection methods for non-Gaussian gravitational wave stochastic backgrounds
- The optimal search for an astrophysical gravitational-wave background
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