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1
Intro
2
Gravitational wave datasets
3
Bayesian inference of GW datasets
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Likelhood computations are too slow
5
Parameter estimation challenges
6
Approaches to faster PE (non-exhausthe list)
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Reduced order quadratures (ROQS) in use
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Outline
9
Numerical integration (quadrature)
10
Do I need a low-order quadrature rule for noisy data?
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Probler Formulation
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Step 1: Compressing the model
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Best approximation space X
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Example basis generation
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Waveform compression application (ex: 1.2040)
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Summary of step 1
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Where are the good points for integrating in X.?
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Empirical interpolation method
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Example: Points for polynomial interpolation integratior
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The ROQ approximation
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Using ROQ
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Building ROQ
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Startup a signal has been detected!
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How much faster?
25
Accelerating tests of GR
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BNS events with third generation observatories
Description:
Explore gravitational wave parameter estimation techniques in this 42-minute lecture by Scott Field from the University of Massachusetts Dartmouth. Delve into the challenges of Bayesian parameter estimation in gravitational wave astronomy and learn about Reduced Order Quadratures (ROQs) as a solution for fast and accurate likelihood evaluations. Discover the key algorithms and software needed to build ROQ rules, and gain insights into their applications for various gravitational wave models. Examine the computational benefits of ROQs, including their exponential convergence and potential to significantly accelerate inference runs. Investigate new challenges and opportunities for ROQs in upcoming detectors, and understand their importance in advancing gravitational wave research.

Gravitational Wave Parameter Estimation with Compressed Likelihood Evaluations

Institute for Pure & Applied Mathematics (IPAM)
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