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  • Publications
    • Analysis of GWTC-3 with fully precessing numerical relativity surrogate models
    • Variational inference for correlated gravitational wave detector network noise
    • Bayesian power spectral density estimation for LISA noise based on P-splines with a parametric boost
    • MorphZ: Enhancing evidence estimation through the Morph approximation
    • Asimov: A framework for coordinating parameter estimation workflows
    • Deep Follow-up for Gravitational-wave Inference: A Case Study with GW151226
    • A follow-up on intermediate-mass black hole candidates in the second LIGO–Virgo observing run with the Bayes Coherence Ratio
    • LIGO–Virgo correlations between mass ratio and effective inspiral spin: testing the active galactic nuclei channel
    • Deep follow-up of GW151226: ordinary binary or low-mass-ratio system?
    • A search for intermediate-mass black holes mergers in the second LIGO--Virgo observing run with the Bayes Coherence Ratio
    • Bayesian inference for compact binary coalescences with <scp>bilby</scp>: validation and application to the first LIGO–Virgo gravitational-wave transient catalogue
  • Slides
    • Example Talk: Recent Work
    • SBI for SGBW
  • Experience
  • Blog
    • Making a personal website workshop
    • Bilby Workshop for NZ Gravity
    • Avi's Pbilby Setup Notes
    • Ozstar Notes
    • Matched Filtering
    • Understanding exoplanet transits
    • Colorblind Palette for Plotting
    • Python Big-O Examples
    • PhD Reports
    • Installing LalSuite from Source

Deep Follow-up for Gravitational-wave Inference: A Case Study with GW151226

April 1, 2023·
Avi vajpeyi
,
Rory smith
,
Eric thrane
· 0 min read
URL DOI
publication
Last updated on April 1, 2023
Authors
Avi vajpeyi
Authors
Rory smith
Authors
Eric thrane
← Asimov: A framework for coordinating parameter estimation workflows April 1, 2023
A follow-up on intermediate-mass black hole candidates in the second LIGO–Virgo observing run with the Bayes Coherence Ratio August 1, 2022 →

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