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on
1
Intro
2
Noise
3
Residual
4
Offsource Method
5
Normalized Periodogram
6
Median
7
Onsource
8
Uncertainty
9
Alternative parametrization
10
Marginalization
11
Student Rayleigh Distribution
12
Onsource Method
13
Caveats
14
Important Sampling
15
Hybrid Approach
16
Alternative Approaches
17
Bayesian Parameter Estimation
18
Summarize
Description:
Explore the impact of power spectral density uncertainty on gravitational-wave parameter estimation in this 46-minute conference talk. Delve into techniques for estimating power spectral density, methods for incorporating uncertainty into parameter estimation frameworks, and the potential systematic biases that can arise when ignoring this uncertainty. Examine the offsource and onsource methods, alternative parametrizations, and approaches like marginalization and important sampling. Gain insights into the context of power spectral density uncertainty within other sources of systematic error in gravitational wave astronomy. Understand the implications for characterizing compact binary coalescences and combining multiple gravitational wave events.

Power Spectral Density Uncertainty and Gravitational-Wave Parameter Estimation

Institute for Pure & Applied Mathematics (IPAM)
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