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Supermassive Black-hole Demographics & Environments With Pulsar Timing Arrays
Published 19 Mar 2019 in astro-ph.GA and gr-qc | (1903.08183v1)
Abstract: Precision timing of large arrays (>50) of millisecond pulsars will detect the nanohertz gravitational-wave emission from supermassive binary black holes within the next ~3-7 years. We review the scientific opportunities of these detections, the requirements for success, and the synergies with electromagnetic instruments operating in the 2020s.
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