First measurement of the Hubble constant from a combined weak lensing and gravitational-wave standard siren analysis

Abstract

We present a new measurement of the Hubble constant ($H_0$) resulting from the first joint analysis of standard sirens with weak gravitational lensing and galaxy clustering observables comprising three two-point correlation functions (3$\times$2pt). For the 3$\times$2pt component of the analysis, we use data from the Dark Energy Survey (DES) Year 3 release. For the standard sirens component, we use data from the Gravitational-Wave Transient Catalog 4.0 released by the LIGO-Virgo-KAGRA (LVK) Collaboration. For GW170817, the only standard siren for which extensive electromagnetic follow-up observations exist, we also use measurements of the host galaxy redshift and inclination angle estimates derived from observations of a superluminal jet from its remnant. Our joint analysis yields $H_0=67.9_{-4.3}^{+4.4}$~km~s${}^{-1}$~Mpc${}^{-1}$, a $6.4\%$ measurement, while improving the DES constraint on the total abundance of matter ${\Omega }_m$ by $22\%$. Removing the jet information degrades the $H_0$ precision to $9.9\%$. The measurement of $H_0$ remains a central problem in cosmology with a multitude of approaches being vigorously pursued in the community aiming to reconcile significantly discrepant measurements at the percent-level. In light of the impending new data releases from DES and LVK, and anticipating much more constraining power from 3$\times$2pt observables using newly commissioned survey instruments, we demonstrate that incorporating standard sirens into the cosmology framework of large cosmic surveys is a viable route towards that goal.

arXiv comment5 pages, 2 figures

References in corpus (45)

• GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
• Advanced Virgo: a 2nd generation interferometric gravitational wave detector
• Cosmic Star Formation History
• Multi-messenger Observations of a Binary Neutron Star Merger
• 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
• Characterization of the LIGO detectors during their sixth science run
• Dark Energy Survey Year 3 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing
• The Dark Energy Camera
• Using gravitational-wave standard sirens
• KiDS-1000 Cosmology: Multi-probe weak gravitational lensing and spectroscopic galaxy clustering constraints
• Superluminal motion of a relativistic jet in the neutron star merger GW170817
• Dark Energy Survey Year 3 Results: Cosmology from Cosmic Shear and Robustness to Data Calibration
• Extracting distribution parameters from multiple uncertain observations with selection biases
• Dark Energy Survey Year 3 Results: Cosmology from Cosmic Shear and Robustness to Modeling Uncertainty
• CosmoSIS: modular cosmological parameter estimation
• 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
• Cosmological parameters from the comparison of peculiar velocities with predictions from the 2M++ density field
• CosmoLike - Cosmological Likelihood Analyses for Photometric Galaxy Surveys
• Groups of Galaxies in the Two Micron All-Sky Redshift Survey
• Constraints on the cosmic expansion history from GWTC-3
• A gravitational-wave measurement of the Hubble constant following the second observing run of Advanced LIGO and Virgo
• Beyond linear galaxy alignments
• Dark Energy Survey Year 3 Results: Photometric Data Set for Cosmology
• Cosmological Inference using Gravitational Wave Standard Sirens: A Mock Data Challenge
• Dark Energy Survey Year 3 Results: Weak Lensing Shape Catalogue
• DES Y3 results: Blending shear and redshift biases in image simulations
• DNF - Galaxy photometric redshift by Directional Neighbourhood Fitting
• Spectral sirens: cosmology from the full mass distribution of compact binaries
• KiDS-Legacy: Cosmological constraints from cosmic shear with the complete Kilo-Degree Survey
• Dark Energy Survey Year 3 Results: Covariance Modelling and its Impact on Parameter Estimation and Quality of Fit
• 2D-FFTLog: Efficient computation of real space covariance matrices for galaxy clustering and weak lensing
• A standard siren measurement of the Hubble constant using gravitational wave events from the first three LIGO/Virgo observing runs and the DESI Legacy Survey
• Dark Energy Survey Year 3 results: Cosmological constraints from galaxy clustering and galaxy-galaxy lensing using the MagLim lens sample
• Binary black holes population and cosmology in new lights: Signature of PISN mass and formation channel in GWTC-3
• Dark Energy Survey Year 3 Results: Optimizing the Lens Sample in Combined Galaxy Clustering and Galaxy-Galaxy Lensing Analysis
• Dark Energy Survey Year 3 Results: Galaxy clustering and systematics treatment for lens galaxy samples
• Does Matter Matter? Using the mass distribution to distinguish neutron stars and black holes
• SPT-3G D1: CMB temperature and polarization power spectra and cosmology from 2019 and 2020 observations of the SPT-3G Main field
• Dark Energy Survey Year 3 Results: High-precision measurement and modeling of galaxy-galaxy lensing
• Dark Energy Survey Year 3 Results: Calibration of Lens Sample Redshift Distributions using Clustering Redshifts with BOSS/eBOSS
• Dark Energy Survey Year 3 results: Magnification modeling and impact on cosmological constraints from galaxy clustering and galaxy-galaxy lensing
• Cross-correlating dark sirens and galaxies: constraints on $H_0$ from GWTC-3 of LIGO-Virgo-KAGRA
• A Comparison of Maps and Power Spectra Determined from South Pole Telescope and Planck Data
• Dark Energy Survey Year 3 Results: Redshift Calibration of the MagLim Lens Sample from the combination of SOMPZ and clustering and its impact on Cosmology
• Be careful in multi-messenger inference of the Hubble constant: A path forward for robust inference