The NANOGrav 11-Year Data Set: Limits on Gravitational Waves from Individual Supermassive Black Hole Binaries

Observations indicate that nearly all galaxies contain supermassive black holes (SMBHs) at their centers. When galaxies merge, their component black holes form SMBH binaries (SMBHBs), which emit low-frequency gravitational waves (GWs) that can be detected by pulsar timing arrays (PTAs). We have sear...

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Published inarXiv.org
Main Authors Aggarwal, K, Arzoumanian, Z, Baker, P T, Brazier, A, Brinson, M R, Brook, P R, Burke-Spolaor, S, Chatterjee, S, Cordes, J M, Cornish, N J, Crawford, F, Crowter, K, Cromartie, H T, DeCesar, M, Demorest, P B, Dolch, T, Ellis, J A, Ferdman, R D, Ferrara, E, Fonseca, E, Garver-Daniels, N, Gentile, P, Hazboun, J S, Holgado, A M, Huerta, E A, Islo, K, Jennings, R, Jones, G, Jones, M L, Kaiser, A R, Kaplan, D L, Kelley, L Z, Key, J S, Lam, M T, Lazio, T J W, Levin, L, Lorimer, D R, Luo, J, Lynch, R S, Madison, D R, McLaughlin, M A, McWilliams, S T, Mingarelli, C M F, C Ng, Nice, D J, Pennucci, T T, Pol, N S, Ransom, S M, Ray, P S, Siemens, X, Simon, J, Spiewak, R, Stairs, I H, Stinebring, D R, Stovall, K, Swiggum, J, Taylor, S R, Turner, J E, Vallisneri, M, R van Haasteren, Vigeland, S J, Witt, C A, Zhu, W W
Format Paper Journal Article
LanguageEnglish
Published Ithaca Cornell University Library, arXiv.org 21.05.2019
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