The curious case of GW200129: interplay between spin-precession inference and data-quality issues
arXiv:2206.11932 · doi:10.1103/PhysRevD.106.104017
Abstract
Measurement of spin-precession in black hole binary mergers observed with gravitational waves is an exciting milestone as it relates to both general relativistic dynamics and astrophysical binary formation scenarios. In this study, we revisit the evidence for spin-precession in GW200129 and localize its origin to data in LIGO Livingston in the 20--50\,Hz frequency range where the signal amplitude is lower than expected from a non-precessing binary given all the other data. These data are subject to known data quality issues as a glitch was subtracted from the detector's strain data. The lack of evidence for spin-precession in LIGO Hanford leads to a noticeable inconsistency between the inferred binary mass ratio and precessing spin in the two LIGO detectors, something not expected from solely different Gaussian noise realizations. We revisit the LIGO Livingston glitch mitigation and show that the difference between a spin-precessing and a non-precessing interpretation for GW200129 is smaller than the statistical and systematic uncertainty of the glitch subtraction, finding that the support for spin-precession depends sensitively on the glitch modeling. We also investigate the signal-to-noise ratio trigger in the less sensitive Virgo detector. Though not influencing the spin-precession studies, the Virgo trigger is grossly inconsistent with the ones in LIGO Hanford and LIGO Livingston as it points to a much heavier system. We interpret the Virgo data in the context of further data quality issues. While our results do not disprove the presence of spin-precession in GW200129, we argue that any such inference is contingent upon the statistical and systematic uncertainty of the glitch mitigation. Our study highlights the role of data quality investigations when inferring subtle effects such as spin-precession for short signals such as the ones produced by high-mass systems.
17 pages, 14 figures, 2 tables. Data release: https://zenodo.org/record/7259655
References in corpus (24)
- Array Programming with NumPy
- Advanced Virgo: a 2nd generation interferometric gravitational wave detector
- Advanced LIGO
- BayesWave: Bayesian Inference for Gravitational Wave Bursts and Instrument Glitches
- Towards models of gravitational waveforms from generic binaries II: Modelling precession effects with a single effective precession parameter
- Multipolar Effective-One-Body Waveforms for Precessing Binary Black Holes: Construction and Validation
- Analysis of spin precession in binary black hole systems including quadrupole-monopole interaction
- BayesLine: Bayesian Inference for Spectral Estimation of Gravitational Wave Detector Noise
- Towards models of gravitational waveforms from generic binaries: A simple approximate mapping between precessing and non-precessing inspiral signals
- Search for gravitational lensing signatures in LIGO-Virgo binary black hole events
- The BayesWave analysis pipeline in the era of gravitational wave observations
- The MBTA Pipeline for Detecting Compact Binary Coalescences in the Third LIGO-Virgo Observing Run
- Characterization of systematic error in Advanced LIGO calibration
- Effective potentials and morphological transitions for binary black-hole spin precession
- qnm: A Python package for calculating Kerr quasinormal modes, separation constants, and spherical-spheroidal mixing coefficients
- Accelerating parameter inference with graphics processing units
- Modeling compact binary signals and instrumental glitches in gravitational wave data
- Precession during merger 1: Strong polarization changes are observationally accessible features of strong-field gravity during binary black hole merger
- Accurate modeling and mitigation of overlapping signals and glitches in gravitational-wave data
- Assessing the model waveform accuracy of gravitational waves
- Daily monitoring of scattered light noise due to microseismic variability at the Virgo interferometer
- Calibration Uncertainty's Impact on Gravitational-Wave Observations
- Evidence of large recoil velocity from a black hole merger signal
- Probing neutron stars with the full pre-merger and post-merger gravitational wave signal from binary coalescences
Cited by in corpus (13)
- Four eccentric mergers increase the evidence that LIGO--Virgo--KAGRA's binary black holes form dynamically
- Neural Importance Sampling for Rapid and Reliable Gravitational-Wave Inference
- Eccentricity or spin precession? Distinguishing subdominant effects in gravitational-wave data
- Data quality up to the third observing run of Advanced LIGO: Gravity Spy glitch classifications
- Tests of general relativity in the nonlinear regime: a parametrized plunge-merger-ringdown gravitational waveform model
- Can gravitational-wave memory help constrain binary black-hole parameters? A LISA case study
- Model exploration in gravitational-wave astronomy with the maximum population likelihood
- Measurability of precession and eccentricity for heavy binary-black-hole mergers
- Identifying glitches near gravitational-wave signals from compact binary coalescences using the Q-transform
- Searching for candidates of coalescing binary black holes formed through chemically homogeneous evolution in GWTC-3
- Distinguishing binary black hole precessional morphologies with gravitational wave observations
- A complete measurement of a black-hole recoil through higher-order gravitational-wave modes
- Theory-agnostic searches for non-gravitational modes in black hole ringdown