A simulated O5-like dark siren analysis shows that host galaxy weighting models become distinguishable only at large detection numbers, with a decisive preference over uniform weighting at about 1000 detections, driven by a few well-localized events.
For the same number of iterations the model built using the LFaB scheme results in an MAE of about 1.5 kcal/mol
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Using gravitational wave dark sirens to choose between host galaxy weighting models
A simulated O5-like dark siren analysis shows that host galaxy weighting models become distinguishable only at large detection numbers, with a decisive preference over uniform weighting at about 1000 detections, driven by a few well-localized events.