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In this study, we investigate the role of the non-linear memory effect in gravitational wave (GW) parameter estimation, particularly we explore its capability to break the degeneracy between luminosity distance and inclination angle in binary coalescence events.
1904
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R. J. Smith, G. Ashton, A. Vajpeyi, and C. Talbot, Massively parallel bayesian inference for transient gravitational-wave astronomy, Monthly Notices of the Royal Astronomical Society 498
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Noise curves used for Simulations in the update of the Observing Scenarios Paper, https://dcc.ligo.org/LIGO-T2000012/public (2022)
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P. Fritschel et al. , Report from the LSC Post-O5 Study Group, Tech. Rep. T2200287 (2022)
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2014
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2015
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2016
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2017
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2017
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2018
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2018
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2018
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2022
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2023
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2023
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2023
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2023
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2023
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2023
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2023
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A# Strain Sensitivity, https://dcc.ligo.org/LIGO-T2300041/public (2023)
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L. S. Collaboration, V. Collaboration, and K. Collaboration, GWTC-3: Compact Binary Coalescences Observed by LIGO and Virgo During the Second Part of the Third Observing Run — Parameter estimation data release, 10.5281/zenodo.8177023 (2023)
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2024
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