Comparing Recent Pulsar Timing Array Results on the Nanohertz Stochastic Gravitational-wave Background
Agazie G, Antoniadis J, Anumarlapudi A, Archibald A, Arumugam P, Arumugam S, Arzoumanian Z, Askew J, Babak S, Bagchi M, Bailes M, Nielsen A, Baker P, Bassa C, Bathula A, Bécsy B, Berthereau A, Bhat N, Blecha L, Bonetti M, Bortolas E, Brazier A, Brook P, Burgay M, Burke-Spolaor S, Burnette R, Caballero R, Cameron A, Case R, Chalumeau A, Champion D, Chanlaridis S, Charisi M, Chatterjee S, Chatziioannou K, Cheeseboro B, Chen S, Chen Z, Cognard I, Cohen T, Coles W, Cordes J, Cornish N, Crawford F, Cromartie H, Crowter K, Curyło M, Cutler C, Dai S, Dandapat S, Deb D, DeCesar M, DeGan D, Demorest P, Deng H, Desai S, Desvignes G, Dey L, Dhanda-Batra N, Di Marco V, Dolch T, Drachler B, Dwivedi C, Ellis J, Falxa M, Feng Y, Ferdman R, Ferrara E, Fiore W, Fonseca E, Franchini A, Freedman G, Gair J, Garver-Daniels N, Gentile P, Gersbach K, Glaser J, Good D, Goncharov B, Gopakumar A, Graikou E, Griessmeier J, Guillemot L, Gültekin K, Guo Y, Gupta Y, Grunthal K, Hazboun J, Hisano S, Hobbs G, Hourihane S, Hu H, Iraci F, Islo K, Izquierdo-Villalba D, Jang J, Jawor J, Janssen G, Jennings R, Jessner A, Johnson A, Jones M, Joshi B, Kaiser A, Kaplan D, Kapur A, Kareem F, Karuppusamy R, Keane E, Keith M, Kelley L, Kerr M, Key J, Kharbanda D, Kikunaga T, Klein T, Kolhe N, Kramer M, Krishnakumar M, Kulkarni A, Laal N, Lackeos K, Lam M, Lamb W, Larsen B, Lazio T, Lee K, Levin Y, Lewandowska N, Littenberg T, Liu K, Liu T, Liu Y, Lommen A, Lorimer D, Lower M, Luo J, Luo R, Lynch R, Lyne A, Ma C, Maan Y, Madison D, Main R, Manchester R, Mandow R, Mattson M, McEwen A, McKee J, McLaughlin M, McMann N, Meyers B, Meyers P, Mickaliger M, Miles M, Mingarelli C, Mitridate A, Natarajan P, Nathan R, Ng C, Nice D, Niţu I, Nobleson K, Ocker S, Olum K, Osłowski S, Paladi A, Parthasarathy A, Pennucci T, Perera B, Perrodin D, Petiteau A, Petrov P, Pol N, Porayko N, Possenti A, Prabu T, Leclere H, Radovan H, Rana P, Ransom S, Ray P, Reardon D, Rogers A, Romano J, Russell C, Samajdar A, Sanidas S, Sardesai S, Schmiedekamp A, Schmiedekamp C, Schmitz K, Schult L, Sesana A, Shaifullah G, Shannon R, Shapiro-Albert B, Siemens X, Simon J, Singha J, Siwek M, Speri L, Spiewak R, Srivastava A, Stairs I, Stappers B, Stinebring D, Stovall K, Sun J, Surnis M, Susarla S, Susobhanan A, Swiggum J, Takahashi K, Tarafdar P, Taylor J, Taylor S, Theureau G, Thrane E, Thyagarajan N, Tiburzi C, Toomey L, Turner J, Unal C, Vallisneri M, van der Wateren E, van Haasteren R, Vecchio A, Krishnan V, Verbiest J, Vigeland S, Wahl H, Wang S, Wang Q, Witt C, Wang J, Wang L, Wayt K, Wu Z, Young O, Zhang L, Zhang S, Zhu X, Zic A, Collaboration T. Comparing Recent Pulsar Timing Array Results on the Nanohertz Stochastic Gravitational-wave Background. The Astrophysical Journal 2024, 966: 105. DOI: 10.3847/1538-4357/ad36be.Peer-Reviewed Original ResearchInternational Pulsar Timing ArrayPulsar timing arraysGravitational-wave backgroundTiming arraysStochastic gravitational-wave backgroundPulsar timing array dataData Release 3Noise parametersRelease 3PulsarSignal-to-noise ratioNoise modelCombination of dataArrayStandard noise modelsAmplitudeParameters
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