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Weitere Publikationen von Autoren mit dem selben Namen

The NANOGrav 12.5-year Data Set: Bayesian Limits on Gravitational Waves from Individual Supermassive Black Hole Binaries, , , , , , , , , und 68 andere Autor(en). (2023)cite arxiv:2301.03608Comment: 20 pages, 12 figures. Submitted to ApJ.The NANOGrav 12.5-year Data Set: Search For An Isotropic Stochastic Gravitational-Wave Background, , , , , , , , , und 51 andere Autor(en). (2020)cite arxiv:2009.04496Comment: 24 pages, 13 figures, 5 tables, 3 appendices. Submitted to The Astrophysical Journal Letters.The effect of differential accretion on the Gravitational Wave Background and the present day MBH Binary population, , und . (2020)cite arxiv:2005.09010Comment: 14 pages, 7 figures.Seeds Don't Sink: Even Massive Black Hole "Seeds" Cannot Migrate to Galaxy Centers Efficiently, , , , , und . (2021)cite arxiv:2101.02727Comment: submitted to MNRAS, comments welcomed.Astrophysics Milestones For Pulsar Timing Array Gravitational Wave Detection, , , , , , , , , und 42 andere Autor(en). (2020)cite arxiv:2010.11950Comment: 14 pages, 7 figures. Abridged abstract presented due to arxiv char limit. Please refer to manuscript for full abstract. Submitted to Nature Astronomy.Simulations of black hole fueling in isolated and merging galaxies with an explicit, multiphase ISM, , , , , , , , , und 2 andere Autor(en). (2022)cite arxiv:2203.14985Comment: 16 pages, 10 figures.Searching For Gravitational Waves From Cosmological Phase Transitions With The NANOGrav 12.5-year dataset, , , , , , , , , und 55 andere Autor(en). (2021)cite arxiv:2104.13930Comment: 13 pages, 4 figures.The NANOGrav 15-year Data Set: Evidence for a Gravitational-Wave Background, , , , , , , , , und 104 andere Autor(en). (2023)cite arxiv:2306.16213Comment: 30 pages, 18 figures. Published in Astrophysical Journal Letters as part of Focus on NANOGrav's 15-year Data Set and the Gravitational Wave Background. For questions or comments, please email comments@nanograv.org.Running Late: Testing Delayed Supermassive Black Hole Growth Models Against the Quasar Luminosity Function, , , , und . (2021)cite arxiv:2109.14647Comment: 11 pages, 6 figures, submitted to MNRAS.