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Comparing merger rate evolution to star formation time delays
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Classroom Contents
Black Hole Astrophysics With Gravitational-Wave Catalogs - IPAM at UCLA
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- 1 Intro
- 2 The origins of LIGO-Virgo's black holes
- 3 Parameter estimation
- 4 Three Astrophysical Lessons
- 5 Effective inspiral spin population distribution
- 6 Comparing merger rate evolution to star formation time delays
- 7 Outlier tests with coarse-grained likelihoods
- 8 Semiparametric population fits in GWTC-3
- 9 Examples of population-level correlations
