Joseph D. Romano, Ph.D.
Affiliations: | Physics | University of Texas at Brownsville, Brownsville, TX, United States |
Area:
GravitationWebsite:
http://www.phys.utb.edu/people/romano.shtmlGoogle:
"Joseph Romano"Mean distance: 12.7 | S | N | B | C | P |
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Publications
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Hazboun JS, Romano JD, Smith TL. (2019) Realistic sensitivity curves for pulsar timing arrays Physical Review D. 100 |
Romano JD, Cornish NJ. (2017) Detection methods for stochastic gravitational-wave backgrounds: a unified treatment. Living Reviews in Relativity. 20: 2 |
Abbott BP, Abbott R, Abbott TD, et al. (2017) Upper Limits on the Stochastic Gravitational-Wave Background from Advanced LIGO's First Observing Run. Physical Review Letters. 118: 121101 |
Abbott BP, Abbott R, Abbott TD, et al. (2016) GW151226: Observation of Gravitational Waves from a 22-Solar-Mass Binary Black Hole Coalescence. Physical Review Letters. 116: 241103 |
Abbott BP, Abbott R, Abbott TD, et al. (2016) GW150914: Implications for the Stochastic Gravitational-Wave Background from Binary Black Holes. Physical Review Letters. 116: 131102 |
Abbott BP, Abbott R, Abbott TD, et al. (2016) Observation of Gravitational Waves from a Binary Black Hole Merger. Physical Review Letters. 116: 061102 |
Abbott BP, Abbott R, Abbott TD, et al. (2016) Binary Black Hole Mergers in the First Advanced LIGO Observing Run Physical Review X. 6: 41015-41015 |
Jenet FA, Romano JD. (2015) Understanding the gravitational-wave Hellings and Downs curve for pulsar timing arrays in terms of sound and electromagnetic waves American Journal of Physics. 83: 635-645 |
Gair JR, Romano JD, Taylor SR. (2015) Mapping gravitational-wave backgrounds of arbitrary polarisation using pulsar timing arrays Physical Review D - Particles, Fields, Gravitation and Cosmology. 92 |
Meacher D, Coughlin M, Morris S, et al. (2015) Mock data and science challenge for detecting an astrophysical stochastic gravitational-wave background with Advanced LIGO and Advanced Virgo Physical Review D - Particles, Fields, Gravitation and Cosmology. 92 |