Frequentist versus Bayesian analyses: Cross-correlation as an (approximate) sufficient statistic for LIGO-Virgo stochastic background searches
arXiv:2012.00907 · doi:10.1103/PhysRevD.103.062003
Abstract
Sufficient statistics are combinations of data in terms of which the likelihood function can be rewritten without loss of information. Depending on the data volume reduction, the use of sufficient statistics as a preliminary step in a Bayesian analysis can lead to significant increases in efficiency when sampling from posterior distributions of model parameters. Here we show that the frequency integrand of the cross-correlation statistic and its variance are approximate sufficient statistics for ground-based searches for stochastic gravitational-wave backgrounds. The sufficient statistics are approximate because one works in the weak-signal approximation and uses measured estimates of the auto-correlated power in each detector. Using analytic and numerical calculations, we prove that LIGO-Virgo's hybrid frequentist-Bayesian parameter estimation analysis is equivalent to a fully Bayesian analysis. This work closes a gap in the LIGO-Virgo literature, and suggests directions for additional searches.
17 pages, 5 figures
References in corpus (34)
- SciPy 1.0--Fundamental Algorithms for Scientific Computing in Python
- Array Programming with NumPy
- Advanced Virgo: a 2nd generation interferometric gravitational wave detector
- Advanced LIGO
- Characterization of the LIGO detectors during their sixth science run
- Science Case for the Einstein Telescope
- Bilby: A user-friendly Bayesian inference library for gravitational-wave astronomy
- Binary Black Hole Population Properties Inferred from the First and Second Observing Runs of Advanced LIGO and Advanced Virgo
- Detecting a stochastic background of gravitational radiation: Signal processing strategies and sensitivities
- Detection methods for stochastic gravitational-wave backgrounds: a unified treatment
- The NANOGrav 11-year Data Set: Pulsar-timing Constraints On The Stochastic Gravitational-wave Background
- Search for the isotropic stochastic background using data from Advanced LIGO's second observing run
- Upper Limits on the Stochastic Gravitational-Wave Background from Advanced LIGO's First Observing Run
- The Sensitivity of Ligo to a Stochastic Background, and its Dependance on the Detector Orientations
- Optimal strategies for gravitational wave stochastic background searches in pulsar timing data
- The stochastic background: scaling laws and time to detection for pulsar timing arrays
- Digging deeper: Observing primordial gravitational waves below the binary black hole produced stochastic background
- Detecting a Stochastic Gravitational Wave Background in the presence of a Galactic Foreground and Instrument Noise
- Analysis of First LIGO Science Data for Stochastic Gravitational Waves
- The Laser Interferometer Space Antenna: Unveiling the Millihertz Gravitational Wave Sky
- Correlated magnetic noise in global networks of gravitational-wave interferometers: observations and implications
- Polarization-based Tests of Gravity with the Stochastic Gravitational-Wave Background
- Subtracting compact binary foreground sources to reveal primordial gravitational-wave backgrounds
- The optimal search for an astrophysical gravitational-wave background
- Parameter Estimation in Searches for the Stochastic Gravitational-Wave Background
- Correlated noise in networks of gravitational-wave detectors: subtraction and mitigation
- Measurement and subtraction of Schumann resonances at gravitational-wave interferometers
- Directional limits on persistent gravitational waves using data from Advanced LIGO's first two observing runs
- Noise-marginalized optimal statistic: A robust hybrid frequentist-Bayesian statistic for the stochastic gravitational-wave background in pulsar timing arrays
- Measuring the primordial gravitational-wave background in the presence of astrophysical foregrounds
- The Photospheric Temperatures of Betelgeuse during the Great Dimming of 2019/2020: No New Dust Required
- Subtraction of correlated noise in global networks of gravitational-wave interferometers
- Detecting a stochastic gravitational-wave background in the presence of correlated magnetic noise
- Robust statistics for deterministic and stochastic gravitational waves in non-Gaussian noise. II: Bayesian analyses
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- Searching for parity violation with the LIGO-Virgo-KAGRA network
- A stochastic search for intermittent gravitational-wave backgrounds
- Deep learning for intermittent gravitational wave signals
- Untargeted Bayesian search of anisotropic gravitational-wave backgrounds through the analytical marginalization of the posterior
- Searching for double-peak and doubly broken gravitational-wave spectra from Advanced LIGO-Virgo's first three observing runs
- Model-independent search for anisotropies in stochastic gravitational-wave backgrounds and application to LIGO-Virgo's first three observing Runs
- Gravitational-wave searches in the era of Advanced LIGO and Virgo
- Background information: a study on the sensitivity of astrophysical gravitational-wave background searches
- Effects of calibration uncertainties on the detection and parameter estimation of isotropic gravitational-wave backgrounds
- Correlation of Gravitational Wave Background Noises and Statistical Loss for Angular Averaged Sensitivity Curves
- Probing the peak of star formation with the stochastic background of binary black hole mergers
- Model-agnostic gravitational-wave background characterization algorithm