Constraining the AGN formation channel for detected black hole binary mergers up to z=1.5 with the Quaia catalogue

Abstract

Statistical analyses based on the spatial correlation between the sky maps of Gravitational Wave (GW) events and the positions of potential host environments are a powerful tool to infer the origin of the black hole binary mergers that have been detected by the LIGO, Virgo, and KAGRA instruments. In this paper, we tighten our previous constraints on the fraction of detected GW events that may have originated from Active Galactic Nuclei (AGN). We consider 159 mergers detected not later than June 1st, 2024, and the all-sky quasar catalogue Quaia. We increase by a factor of 5.3 and 114 the number of considered GW sources and AGN respectively, also extending our analysis from redshift $0.3$ to $1.5$. This is possible thanks to the uniformity of the AGN catalogue and its high level of completeness, which we estimate as a function of redshift and luminosity. We find at a 95 per cent credibility level that un-obscured AGN with a bolometric luminosity higher than $10^{44.5}{\mathrm{erg}\mathrm{s}}^{-1}$ ($10^{45}{\mathrm{erg}\mathrm{s}}^{-1}$) do not contribute to more than the 21 (11) per cent of the detected GW events.

12 pages, 7 figures, 3 tables

References in corpus (52)

• SciPy 1.0--Fundamental Algorithms for Scientific Computing in Python
• Array Programming with NumPy
• Astropy: A Community Python Package for Astronomy
• Planck 2015 results. XIII. Cosmological parameters
• GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
• The Astropy Project: Building an inclusive, open-science project and status of the v2.0 core package
• Advanced Virgo: a 2nd generation interferometric gravitational wave detector
• Gaia Data Release 3: Summary of the content and survey properties
• Advanced LIGO
• The Zwicky Transient Facility: System Overview, Performance, and First Results
• The Nucleosynthetic Signature of Population III
• Spectral Energy Distributions and Multiwavelength Selection of Type 1 Quasars
• Bilby: A user-friendly Bayesian inference library for gravitational-wave astronomy
• An Observational Determination of the Bolometric Quasar Luminosity Function
• The Zwicky Transient Facility: Science Objectives
• Toward the Standard Population Synthesis Model of the X-Ray Background: Evolution of X-Ray Luminosity and Absorption Functions of Active Galactic Nuclei Including Compton-Thick Populations
• Binary Black Hole Mergers from Globular Clusters: Masses, Merger Rates, and the Impact of Stellar Evolution
• Computationally efficient models for the dominant and sub-dominant harmonic modes of precessing binary black holes
• Rapid and Bright Stellar-mass Binary Black Hole Mergers in Active Galactic Nuclei
• The Sloan Digital Sky Survey Quasar Catalog: Sixteenth Data Release
• A torque formula for non-isothermal Type I planetary migration - I. Unsaturated horseshoe drag
• Rapid Bayesian position reconstruction for gravitational-wave transients
• Formation and Evolution of Compact Object Binaries in AGN Disks
• The Effect of Pair-Instability Mass Loss on Black Hole Mergers
• unWISE: unblurred coadds of the WISE imaging
• The incidence of obscuration in active galactic nuclei
• Are merging black holes born from stellar collapse or previous mergers?
• Updating quasar bolometric luminosity corrections
• Hierarchical Black Hole Mergers in Active Galactic Nuclei
• Dynamics of stellar black holes in young star clusters with different metallicities - II. Black hole-black hole binaries
• Migration Traps in Disks Around Supermassive Black Holes
• Evolution of the AGN UV luminosity function from redshift 7.5
• A Catalog of Quasar Properties from Sloan Digital Sky Survey Data Release 16
• AGN Disks Harden the Mass Distribution of Stellar-mass Binary Black Hole Mergers
• Escape speed of stellar clusters from multiple-generation black-hole mergers in the upper mass gap
• Aligning Nuclear Cluster Orbits with an Active Galactic Nucleus Accretion Disk
• The most ordinary formation of the most unusual double black hole merger
• A light in the dark: searching for electromagnetic counterparts to black hole-black hole mergers in LIGO/Virgo O3 with the Zwicky Transient Facility
• Review of the Advanced LIGO gravitational wave observatories leading to observing run four
• Do LIGO/Virgo black hole mergers produce AGN flares? The case of GW190521 and prospects for reaching a confident association
• Black Hole Binary Formation in AGN Discs: From Isolation to Merger
• Formation channels of single and binary stellar-mass black holes
• Quaia, the Gaia-unWISE Quasar Catalog: An All-Sky Spectroscopic Quasar Sample
• unWISE Coadds: The Five-year Data Set
• Gravitational-Wave Localization Alone Probes AGN Origin of Stellar-Mass Black Hole Mergers
• Black hole mergers of AGN origin in LIGO/Virgo's O1-O3a observing periods
• Gas dynamical friction as a binary formation mechanism in AGN discs
• The Effect of Thermal Torques on AGN Disc Migration Traps and Gravitational Wave Populations
• Aligning Retrograde Nuclear Cluster Orbits with an Active Galactic Nucleus Accretion Disc
• The most luminous AGN do not produce the majority of the detected stellar-mass black hole binary mergers in the local Universe
• Localization of Binary Black-Hole Mergers with Known Inclination
• Ancestral Black Holes of Binary Merger GW190521

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• The Science of the Einstein Telescope
• Evidence of a fraction of LIGO/Virgo/KAGRA events coming from active galactic nuclei
• The origin channels of hierarchical binary black hole mergers in the LIGO-Virgo-KAGRA O1, O2, and O3 runs
• Not all roads lead to merger: AGN disc properties influence the interactions of highly unequal mass black holes
• The Use of Binary Black Holes Merging in AGN Disks for Hubble Constant Measurements
• Tracing the high-z cosmic web with Quaia: catalogues of voids and clusters in the quasar distribution