StAGE: Stellar Archaeology-driven Galaxy Evolution II. Binary Black Hole Mergers in Quiescent Galaxies and their Star-forming Progenitors
astro-ph.GA, astro-ph.CO
Submitted: 2026-09-21
Updated: 2026-09-21
Comments: 53 pages, 18 figures
Code: https://github.com/marcasedda/BPOP
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Observation of Gravitational Waves from a Binary Black Hole Merger
- Characterization of the LIGO detectors during their sixth science run
- Gravitational-wave astronomy requires population-informed parameter estimation
- Advanced Virgo: a 2nd generation interferometric gravitational wave detector
- Overview of KAGRA: Detector design and construction history
- Binary Black Hole Population Properties Inferred from the First and Second Observing Runs of Advanced LIGO and Advanced Virgo
- Population Properties of Compact Objects from the Second LIGO-Virgo Gravitational-Wave Transient Catalog
- The population of merging compact binaries inferred using gravitational waves through GWTC-3
- Compact Binary Coalescences: Astrophysical Processes and Lessons Learned
- Physical Models for the Astrophysical Population of Black Holes: Application to the Bump in the Mass Distribution of Gravitational Wave Sources
- The first gravitational-wave source from the isolated evolution of two 40-100 Msun stars
- Binary black hole mergers: formation and populations
- One Channel to Rule Them All? Constraining the Origins of Binary Black Holes using Multiple Formation Pathways
- What You Don't Know Can Hurt You: Use and Abuse of Astrophysical Models in Gravitational-wave Population Analyses
- Exploring the evolution of gravitational-wave emitters with efficient emulation: Constraining the origins of binary black holes using normalising flows
- Seeking Spinning Subpopulations of Black Hole Binaries via Iterative Density Estimation
- Compactness Peaks and Subpopulations: Probing Stellar Physics and Formation Channels of Merging Binary Black Holes
- Inferring black hole formation channels in GWTC-4.0 via parametric mass-spin correlations derived from first principles
- Probing Spin-Orbit Resonances with the Binary Black Hole Population
- Binary Population and Spectral Synthesis Version 2.1: construction, observational verification and new results
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