| ... | @@ -13,6 +13,11 @@ weights = np.square(bilby_posterior['mass_1']) / bilby_posterior['chirp_mass'] |
... | @@ -13,6 +13,11 @@ weights = np.square(bilby_posterior['mass_1']) / bilby_posterior['chirp_mass'] |
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* Additionally, the `phi_1` and `phi_2` figures also show a discrepancy. In the telecon [190813](https://git.ligo.org/lscsoft/bilby_pipe/wikis/O3-review/minutes/190813), Colm demonstrated this was also due to the waveforms interface by again comparing results from O3 L.I. runs.
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* Additionally, the `phi_1` and `phi_2` figures also show a discrepancy. In the telecon [190813](https://git.ligo.org/lscsoft/bilby_pipe/wikis/O3-review/minutes/190813), Colm demonstrated this was also due to the waveforms interface by again comparing results from O3 L.I. runs.
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## Distance
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* The individual MCMC and Nest runs from `LALInference` will likely not have been corrected for the distance bug, see https://git.ligo.org/lscsoft/lalsuite/merge_requests/780.
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This will make the LI distance closer by a few percent and introduce a small bias in source-frame masses.
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## Comparison with LALInference
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## Comparison with LALInference
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We compare all results to LALInference Nest and MCMC runs using the IMRPhenomPv2 analyses performed for GWTC1.
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We compare all results to LALInference Nest and MCMC runs using the IMRPhenomPv2 analyses performed for GWTC1.
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