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Single Sources in the Low-Frequency Gravitational Wave Sky: properties and time to detection by pulsar timing arrays
Luke Zoltan Kelley, Laura Blecha, Lars Hernquist +2
We calculate the properties, occurrence rates and detection prospects of individually resolvable 'single sources' in the low frequency gravitational wave (GW) spectrum. Our simulat…
Testing the binary hypothesis: pulsar timing constraints on supermassive black hole binary candidates
A. Sesana, Z. Haiman, B. Kocsis +1
The advent of time domain astronomy is revolutionizing our understanding of the Universe. Programs such as the Catalina Real-time Transient Survey (CRTS) or the Palomar Transient F…
The Gravitational Wave Background from Massive Black Hole Binaries in Illustris: spectral features and time to detection with pulsar timing arrays
Luke Zoltan Kelley, Laura Blecha, Lars Hernquist +2
Pulsar Timing Arrays (PTA) around the world are using the incredible consistency of millisecond pulsars to measure low frequency gravitational waves from (super)Massive Black Hole…