A neutron star in a compact binary generates relativistic Alfven wings that carry most of the intersected electromagnetic power and may produce periodic pulsar-like emission.
Nakar , journal volume 886 , pages 1 ( year 2020 ), 1912.05659
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Baselines of 8-11 ms light travel time for two CE detectors provide a reasonable compromise for BBH sky localization, with third detectors eliminating multimodality for most or all events.
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Alfven-winged pulsar
A neutron star in a compact binary generates relativistic Alfven wings that carry most of the intersected electromagnetic power and may produce periodic pulsar-like emission.
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Not too close! Evaluating the impact of the baseline on the localization of binary black holes by next-generation gravitational-wave detectors
Baselines of 8-11 ms light travel time for two CE detectors provide a reasonable compromise for BBH sky localization, with third detectors eliminating multimodality for most or all events.