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pro vyhledávání: '"Deng, Xihao"'
Autor:
Arzoumanian, Zaven, Brazier, Adam, Burke-Spolaor, Sarah, Chamberlin, Sydney, Chatterjee, Shami, Christy, Brian, Cordes, Jim, Cornish, Neil, Demorest, Paul, Deng, Xihao, Dolch, Tim, Ellis, Justin, Ferdman, Rob, Fonseca, Emmanuel, Garver-Daniels, Nate, Jenet, Fredrick, Jones, Glenn, Kaspi, Vicky, Koop, Michael, Lam, Michael, Lazio, Joseph, Levin, Lina, Lommen, Andrea, Lorimer, Duncan, Luo, Jin, Lynch, Ryan, Madison, Dustin, McLaughlin, Maura, McWilliams, Sean, Mingarelli, Chiara, Nice, David, Palliyaguru, Nipuni, Pennucci, Tim, Ransom, Scott, Sampson, Laura, Sanidas, Sotiris, Sesana, Alberto, Siemens, Xavier, Simon, Joseph, Stairs, Ingrid, Stinebring, Dan, Stovall, Kevin, Swiggum, Joseph, Taylor, Stephen, Vallisneri, Michele, van Haasteren, Rutger, Wang, Yan, Zhu, Weiwei
We compute upper limits on the nanohertz-frequency isotropic stochastic gravitational wave background (GWB) using the 9-year data release from the North American Nanohertz Observatory for Gravitational Waves (NANOGrav) collaboration. We set upper lim
Externí odkaz:
http://arxiv.org/abs/1508.03024
Autor:
Deng, Xihao
Publikováno v:
Physical Review D, 90, 104029, 2014
Gravitational wave background results from the superposition of gravitational waves generated from all sources across the Universe. Previous efforts on detecting such a background with pulsar timing arrays assume it is an isotropic Gaussian backgroun
Externí odkaz:
http://arxiv.org/abs/1410.6441
Autor:
Deng, Xihao
Publikováno v:
Physical Review D, 90, 024020, 2014
Gravitational wave burst is a catch-all category for signals whose durations are shorter than the observation period. We apply a method new to gravitational wave data analysis --- Bayesian non-parameterics --- to the problem of gravitational wave det
Externí odkaz:
http://arxiv.org/abs/1404.0663
Autor:
Deng, Xihao, Finn, Lee Samuel
Pulsar timing arrays act to detect gravitational waves by observing the small, correlated effect the waves have on pulse arrival times at Earth. This effect has conventionally been evaluated assuming the gravitational wave phasefronts are planar acro
Externí odkaz:
http://arxiv.org/abs/1008.0320
Akademický článek
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Autor:
Deng, Xihao
Publikováno v:
AIP Conference Proceedings; 7/25/2012, Vol. 1467 Issue 1, p231-234, 4p, 1 Graph