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Reply to ‘Presence of a fundamental acceleration scale in galaxies’ and ‘A common Milgromian acceleration scale in nature’

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Fig. 1: Analyses of the χ2ν CDF.
Fig. 2: Posterior probability distributions of a0.

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Acknowledgements

D.C.R. and V.M. thank CNPq and FAPES (Brazil) for partial financial support. A.D.P. was supported by the Chinese Academy of Sciences and by the President’s International Fellowship Initiative, grant number 2017 VMA0044. Z.D. thanks the Ministry of Science, Research and Technology of Iran for financial support.

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Authors and Affiliations

  1. Center for Astrophysics and Cosmology, CCE, Federal University of Espírito Santo, Vitória, Brazil

    Davi C. Rodrigues & Valerio Marra

  2. Department of Physics, CCE, Federal University of Espírito Santo, Vitória, Brazil

    Davi C. Rodrigues & Valerio Marra

  3. Dipartamento di Fisica e Astronomia, Università di Catania, Catania, Italy

    Antonino Del Popolo

  4. Institute of Modern Physics, Chinese Academy of Sciences, Lanzhou, People’s Republic of China

    Antonino Del Popolo

  5. INFN sezione di Catania, Catania, Italy

    Antonino Del Popolo

  6. Department of Physics, Bu-Ali Sina University, Hamedan, Iran

    Zahra Davari

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  1. Davi C. Rodrigues
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  2. Valerio Marra
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  3. Antonino Del Popolo
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  4. Zahra Davari
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Correspondence to Davi C. Rodrigues or Valerio Marra.

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Rodrigues, D.C., Marra, V., Del Popolo, A. et al. Reply to ‘Presence of a fundamental acceleration scale in galaxies’ and ‘A common Milgromian acceleration scale in nature’. Nat Astron 2, 927–929 (2018). https://doi.org/10.1038/s41550-018-0614-x

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