Neural posterior estimation shows a two-misaligned-L ET network yields better sky and volume localization for high-redshift massive BBHs than triangular ET, with fewer multimodalities, though luminosity distance estimates are less precise.
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Comparing next-generation detector configurations for high-redshift gravitational wave sources with neural posterior estimation
Neural posterior estimation shows a two-misaligned-L ET network yields better sky and volume localization for high-redshift massive BBHs than triangular ET, with fewer multimodalities, though luminosity distance estimates are less precise.