Survey continuation yields FRB20110220A, RRAT J0404+53, new data on J2028+28, and evidence that single-pulse detection rates vary with Galactic coordinates, implying a faint Galactic population.
R., Portegies Zwart, S
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Nemesis couples global and local astrophysical simulations to match direct N-body results while scaling efficiently when cores exceed the number of planetary systems.
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The Northern High Time Resolution Universe pulsar survey: III. Single-pulse search continuation, follow-up observations, and initial results
Survey continuation yields FRB20110220A, RRAT J0404+53, new data on J2028+28, and evidence that single-pulse detection rates vary with Galactic coordinates, implying a faint Galactic population.
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Nemesis: A Multi-Scale, Multi-Physics Algorithm for Astrophysics
Nemesis couples global and local astrophysical simulations to match direct N-body results while scaling efficiently when cores exceed the number of planetary systems.