Detection of eccentric supermassive black hole binaries with pulsar timing arrays: Signal-to-noise ratio calculations

Authors

E. A. Huerta
Sean T. McWilliams
Jonathan R. Gair
Stephen R. Taylor

Author ORCID Identifier

N/A

https://orcid.org/0000-0003-2397-8290

https://orcid.org/0000-0002-1671-3668

https://orcid.org/0000-0003-0264-1453

Document Type

Article

Publication Date

2015

Digital Commons Citation

Huerta, E. A.; McWilliams, Sean T.; Gair, Jonathan R.; and Taylor, Stephen R., "Detection of eccentric supermassive black hole binaries with pulsar timing arrays: Signal-to-noise ratio calculations" (2015). Faculty & Staff Scholarship. 123.
https://researchrepository.wvu.edu/faculty_publications/123

Source Citation

Huerta, E. A., McWilliams, Sean T., Gair, Jonathan R., & Taylor, Stephen R. (2015). Detection Of Eccentric Supermassive Black Hole Binaries With Pulsar Timing Arrays: Signal-To-Noise Ratio Calculations. Physical Review D - Particles, Fields, Gravitation, and Cosmology, 92(6). http://doi.org/10.1103/PhysRevD.92.063010