Titlebook: Wahrscheinlichkeitsrechnung und Statistik; Robert Hafner Book 1989 Springer-Verlag, Wien 1989 Mathematische Statistik.Statistik.Testtheori

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coherent superposition of the cosmic population of SMBHBs is expected to form a diffusive GW background, which has yet to be detected, cf. Hellings and Downs (1983), Rajagopal and Romani (.), Wyithe and Loeb (.), Sesana et al. (.), Jaffe and Backer (.), Jenet et al. (.), Sesana et al. (.), van Haast

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Robert Hafnerc backgrounds. Where appropriate, model probability density functions for the data under hypotheses about signal strength are developed. These procedures are then applied to existing data to demonstrate algorithm performance and limitations. Finally, the sensitivities possible in future- generation

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Robert Hafner) simulations. We extensively test our approach on mock PTA datasets, and find that the Bayesian inference method has significant benefits over currently proposed counterparts. We show the importance of characterising all red noise components in pulsar timing noise by demonstrating that the presence

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Robert Hafnerrk. The discovery verified Einstein’s century-old prediction and enabled for the first time the direct detection of a black hole and a black hole binary system. It also opened the new window of gravitational wave astronomy to the Universe, which until then could be observed only through electromagne

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Robert Hafnerotion functions: walking, sitting, holding and lifting, are proposed, their static balancing methods and approaches, comparative numerical analysis, advantages and disadvantages are given. In addition, the proposed approaches and solutions are universal and can be used in the design of assistive dev

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Robert Hafnerided in this book. This is also true for the tidal effects, removed by a tidal reduction, while, on the other hand, the removal of the instrumental drift can be considered truly a correction. The ultimate accuracy of the anomaly values is affected by both the observations and the reductions.

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Robert Hafnerd geoid changes, such as positive geoid height rates in Laurentia and Fennoscandia related to glacial isostatic adjustments, and negative rates in Greenland and West Antarctica, as a result of mass losses due to ice-sheet melting. Also, the upper mantle viscosity in Fennoscandia is determined by the

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