Standard Siren Speeds: Improving velocities in gravitational-wave measurements of
arXiv:1909.00587 · doi:10.1093/mnras/staa049
Abstract
We re-analyze data from the gravitational-wave event GW170817 and its host galaxy NGC4993 to demonstrate the importance of accurate total and peculiar velocities when measuring the Hubble constant using this nearby Standard Siren. We show that a number of reasonable choices can be made to estimate the velocities for this event, but that systematic differences remain between these measurements depending on the data used. This leads to significant changes in the Hubble constant inferred from GW170817. We present Bayesian Model Averaging as one way to account for these differences, and obtain . Adding additional information on the viewing angle from high resolution imaging of the radio counterpart refines this to . During this analysis we also present an alternative Bayesian model for the posterior on from Standard Sirens that works more closely with observed quantities from redshift and peculiar velocity surveys. Our results more accurately capture the true uncertainty on the total and peculiar velocities of NGC4993 and show that exploring how well different datasets characterize galaxy groups and the velocity field in the local Universe could improve this measurement further. These considerations impact any low-redshift distance measurement, and the improvements we suggest here can also be applied to standard candles like type Ia supernovae. GW170817 is particularly sensitive to peculiar velocity uncertainties because it is so close. For future standard siren measurements the importance of this error will decrease as (a) we will measure more distant standard sirens, and (b) the random direction of peculiar velocities will average out with more detections.
arXiv comment13 pages, 5 figures. Updated to match accepted version in MNRAS; textual changes only (results/figures unchanged)
References in corpus (39)
- emcee: The MCMC Hammer
- The Sloan Digital Sky Survey: Technical Summary
- GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
- Advanced Virgo: a 2nd generation interferometric gravitational wave detector
- Multi-messenger Observations of a Binary Neutron Star Merger
- Advanced LIGO
- Large Magellanic Cloud Cepheid Standards Provide a 1% Foundation for the Determination of the Hubble Constant and Stronger Evidence for Physics Beyond LambdaCDM
- A gravitational-wave standard siren measurement of the Hubble constant
- The 6dF Galaxy Survey: Final Redshift Release (DR3) and Southern Large-Scale Structures
- The Carnegie-Chicago Hubble Program. VIII. An Independent Determination of the Hubble Constant Based on the Tip of the Red Giant Branch
- The 2MASS Redshift Survey - Description and Data Release
- Cosmicflows-3
- A 2 per cent Hubble constant measurement from standard sirens within 5 years
- Our Peculiar Motion Away from the Local Void
- A Nested Sampling Algorithm for Cosmological Model Selection
- The SBF Survey of Galaxy Distances. II. Local and Large-Scale Flows
- 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
- Groups of Galaxies in the Two Micron All-Sky Redshift Survey
- A standard siren measurement of the Hubble constant from GW170817 without the electromagnetic counterpart
- The 2M++ galaxy redshift catalogue
- Galaxy Groups within 3500 km s
- Expanding Confusion: common misconceptions of cosmological horizons and the superluminal expansion of the Universe
- Galaxy groups and clouds in the Local (z~0.01) universe
- The Distance to NGC 4993: The Host Galaxy of the Gravitational-wave Event GW170817
- A Precise Distance to the Host Galaxy of the Binary Neutron Star Merger GW170817 Using Surface Brightness Fluctuations
- Galaxy Groups: A 2MASS Catalog
- The 6dF Galaxy Survey: The Near-Infrared Fundamental Plane of Early-Type Galaxies
- The 6dF Galaxy Survey: Bulk Flows on Mpc scales
- The peculiar velocity field up to by forward-modeling Cosmicflows-3 data
- Distance and properties of NGC 4993 as the host galaxy of a gravitational wave source, GW170817
- Can redshift errors bias measurements of the Hubble Constant?
- Unbiased Hubble constant estimation from binary neutron star mergers
- Improving cosmological parameter estimation with the future gravitational-wave standard siren observation from the Einstein Telescope
- An Unbiased Estimator of Peculiar Velocity with Gaussian Distributed Errors for Precision Cosmology
- 2MTF - VII. 2MASS Tully-Fisher survey final data release: distances for 2,062 nearby spiral galaxies
- Bulk flow and shear in the local Universe: 2MTF and COSMICFLOWS-3
- Bayesian Model Averaging in Astrophysics: A Review
- Bulk flow in the combined 2MTF and 6dFGSv surveys
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- Cosmology with the Laser Interferometer Space Antenna
- The CosmoVerse White Paper: Addressing observational tensions in cosmology with systematics and fundamental physics
- A buyer's guide to the Hubble Constant
- Cosmological Inference using Gravitational Wave Standard Sirens: A Mock Data Challenge
- Accurate precision Cosmology with redshift unknown gravitational wave sources
- A statistical standard siren measurement of the Hubble constant from the LIGO/Virgo gravitational wave compact object merger GW190814 and Dark Energy Survey galaxies
- The Pantheon+ Analysis: Evaluating Peculiar Velocity Corrections in Cosmological Analyses with Nearby Type Ia Supernovae
- Velocity correction for Hubble constant measurements from standard sirens
- Forecast for cosmological parameter estimation with gravitational-wave standard sirens from the LISA-Taiji network
- The Sloan Digital Sky Survey Peculiar Velocity Catalogue
- The Challenges Ahead for Multimessenger Analyses of Gravitational Waves and Kilonova: a Case Study on GW190425
- The Impact of Peculiar Velocities on the Estimation of the Hubble Constant from Gravitational Wave Standard Sirens
- Constraining the Hubble constant to a precision of about 1% using multi-band dark standard siren detections
- Spherical symmetry in the kilonova AT2017gfo/GW170817
- Systematic uncertainty of standard sirens from the viewing angle of binary neutron star inspirals
- Constraining the cosmological parameters using gravitational wave observations of massive black hole binaries and statistical redshift information
- Constrained realizations of 2MRS density and peculiar velocity fields: growth rate and local flow
- Target Selection for the DESI Peculiar Velocity Survey
- Peculiar velocities in the local Universe: comparison of different models and the implications for and dark matter
- Measurements of the Hubble Constant with a Two Rung Distance Ladder: Two Out of Three Ain't Bad
- Cosmography with next-generation gravitational wave detectors
- Exploiting the Einstein Telescope to solve the Hubble tension
- Probing gravity and growth of structure with gravitational waves and galaxies' peculiar velocity
- The binary-host connection: astrophysics of gravitational wave binaries from their host galaxy properties
- The late afterglow of GW170817/GRB170817A: a large viewing angle and the shift of the Hubble constant to a value more consistent with the local measurements
- Does non-stationary noise in LIGO and Virgo affect the estimation of ?
- Measuring the Hubble constant with kilonovae using the Expanding Photosphere Method
- Using Gray Sirens to Resolve the Hubble-Lemaître Tension
- Emergence hour-by-hour of -process features in the kilonova AT2017gfo
- Multimessenger astronomy with a kHz-band gravitational-wave observatory
- Standard siren cosmology in the era of the 2.5-generation ground-based gravitational wave detectors: bright and dark sirens of LIGO Voyager and NEMO
- Constraining properties of neutron star merger outflows with radio observations
- Moving gravitational wave sources at cosmological distances: Impact on the measurement of the Hubble constant
- The luminosity functions of kilonovae from binary neutron star mergers under different equation of states
- Direct geometrical measurement of the Hubble constant from galaxy parallax: predictions for the Vera C. Rubin Observatory and Nancy Grace Roman Space Telescope
- Impact of calibration uncertainties on Hubble constant measurements from gravitational-wave sources
- Cosmic Cartography II: completing galaxy catalogs for gravitational-wave cosmology
- Considering light-matter interactions in the Friedmann equations
- Biases in velocity reconstruction: investigating the effects on growth rate and expansion measurements in the local universe
- Mapping the cosmic expansion history from LIGO-Virgo-KAGRA in synergy with DESI and SPHEREx
- The Luminosity of the Darkness: Schechter function in dark sirens
- Listening Across the Cosmic Time: Standard Sirens from Ground- and Space-Based Missions in the Next Decade