A Hubble constant estimation with dark standard sirens and galaxy cluster catalogues
arXiv:2505.14077 · doi:10.1093/mnras/staf1432
Abstract
In this paper, we explore the possibility of using galaxy cluster catalogues to provide redshift support for a gravitational-wave dark standard siren measurement of the Hubble constant . We adapt the cosmology inference pipeline gwcosmo to handle galaxy cluster catalogues. Together with binary black holes from the GWTC-3, we use galaxy cluster data from the PSZ2 and the eRASS catalogues. With these catalogues, we obtain and respectively, which demonstrates improvements on precision by factors of 10% and 38% respectively over the traditional galaxy catalogue result. This exploratory work paves the way towards precise and accurate cosmography making use of distant compact binary mergers from upcoming observing runs of the LIGO-Virgo-KAGRA detector network and future gravitational-wave observatories.
References in corpus (35)
- Cosmic Star Formation History
- GW190814: Gravitational Waves from the Coalescence of a 23 M Black Hole with a 2.6 M Compact Object
- Ellipsoidal collapse and an improved model for the number and spatial distribution of dark matter haloes
- GWTC-3: Compact Binary Coalescences Observed by LIGO and Virgo During the Second Part of the Third Observing Run
- A gravitational-wave standard siren measurement of the Hubble constant
- Using gravitational-wave standard sirens
- Open data from the first and second observing runs of Advanced LIGO and Advanced Virgo
- Open data from the third observing run of LIGO, Virgo, KAGRA and GEO
- 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
- Measuring a cosmological distance-redshift relationship using only gravitational wave observations of binary neutron star coalescences
- 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
- A standard siren measurement of the Hubble constant from GW170817 without the electromagnetic counterpart
- A Future Percent-Level Measurement of the Hubble Expansion at Redshift 0.8 With Advanced LIGO
- Cosmological Inference using Gravitational Wave Standard Sirens: A Mock Data Challenge
- Accurate precision Cosmology with redshift unknown gravitational wave sources
- The Observational Mass Function of Nearby Galaxy Clusters
- Cosmology in the dark: On the importance of source population models for gravitational-wave cosmology
- A statistical standard siren measurement of the Hubble constant from the LIGO/Virgo gravitational wave compact object merger GW190814 and Dark Energy Survey galaxies
- Spectral sirens: cosmology from the full mass distribution of compact binaries
- Measuring the distance-redshift relation with the cross-correlation of gravitational wave standard sirens and galaxies
- GLADE+: An Extended Galaxy Catalogue for Multimessenger Searches with Advanced Gravitational-wave Detectors
- Large-scale mass distribution in the Illustris simulation
- 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
- Binary black holes population and cosmology in new lights: Signature of PISN mass and formation channel in GWTC-3
- The Hitchhiker's guide to the galaxy catalog approach for gravitational wave cosmology
- Gravitational wave cosmology with extreme mass-ratio inspirals
- Caught in the cosmic web: Environmental effect on halo concentrations, shape, and spin
- The redshift dependence of black hole mass distribution: Is it reliable for standard sirens cosmology?
- Cosmography with next-generation gravitational wave detectors
- Gravitational-wave dark siren cosmology systematics from galaxy weighting
- Testing the nature of gravitational wave propagation using dark sirens and galaxy catalogues
- Bayesian framework to infer the Hubble constant from the cross-correlation of individual gravitational wave events with galaxies
- Beyond Gaps and Bumps: Spectral Siren Cosmology with Non-Parametric Population Models
- Gravitational Wave Cosmology