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Atrio-Barandela, F., Kashlinsky, A., Ebeling, H., Fixsen, D.J. and Kocevski, D. Probing the Dark Flow Signal in WMAP 9 yr and PLANCK Cosmic Microwave Background Maps. arXiv:1411.4180v2 [astro-ph.CO] 22 Jul 2015.
https://arxiv.org/abs/1411.4180

has been cited by the following article:

  • TITLE: The Cause of the Allais Effect Solved

    AUTHORS: Bjarne Lorenzen

    KEYWORDS: Allais Effect, Anisotropic Acceleration, Dark Flow

    JOURNAL NAME: International Journal of Astronomy and Astrophysics, Vol.7 No.2, June 8, 2017

    ABSTRACT: An Anisotropic Dark Flow Acceleration can solve the cause of the Allais Effect [1]. This claim is based on a kinematic analysis of 21 Allais Effect measurements. All measurements (without exception) substantiate that the Allais Effect is consistent with anisotropic acceleration and that the acceleration is directed in the same direction as Dark Flow. So far, Allais Effect measurements have taken place blindfolded. Now, it is possible to calculate and predict when and where the Allais Effect can be confirmed, and of course also predict where and why no effect can be confirmed. In addition, it is now also possible to calculate how strong anomalies can be expected, and even whether the effect can be measured before or after the eclipse reaches the maximum. Still different pendulums are the most effective instrument to use. The reason why such strange devices are the best option is also no longer a mystery. This new theory also uncovers why advanced instruments can’t be used successfully, which also explains why such significant acceleration could have been hidden for such a long time. The exact magnitude of the anisotropic acceleration is calculated to be around 35 μGal (3.5e−7 m/s2), and not much deviation must be expected in the years to come.