By accident, we performed some runs with fiducial parameters that are a very bad fit to the actual signal.
By accident, we performed some runs with fiducial parameters that are a very bad fit to the actual signal (the mass and spin for one of the NSBH simulations was used instead of the neutron star masses).
In this case, we found that the rejection sampling efficiency was very small with large mismatches.
In this case, we found that the rejection sampling efficiency was very small with large mismatches.
The corresponding analysis can be found at `/home/sylvia.biscoveanu/bilby_pipe/runs/review_test/O4/fiducial_bns_PhenomTidal_take2/outdir_dynesty_relbin_medSpin_precessing_cal`.
The corresponding analysis can be found at `/home/sylvia.biscoveanu/bilby_pipe/runs/review_test/O4/fiducial_bns_PhenomTidal_take2/outdir_dynesty_relbin_medSpin_precessing_cal`.
