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Reply to: Overconfidence in Bayesian analyses of galaxy rotation curves

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The Original Article was published on 27 January 2020

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References

  1. Cameron, E., Angus, G. W. & Burgess, J. M. Overconfidence in Bayesian analyses of galaxy rotation curves. Nat. Astron. https://doi.org/10.1038/s41550-019-0998-2 (2020).

  2. Rodrigues, D. C., Marra, V., Del Popolo, A. & Davari, Z. Absence of a fundamental acceleration scale in galaxies. Nat. Astron. 2, 668–672 (2018).

    Article  ADS  Google Scholar 

  3. Frigerio Martins, C. & Salucci, P. Analysis of rotation curves in the framework of R n gravity. Mon. Not. R. Astron. Soc. 381, 1103–1108 (2007).

    Article  ADS  Google Scholar 

  4. Gentile, G., Famaey, B. & de Blok, W. J. G. THINGS about MOND. Astron. Astrophys. 527, A76 (2011).

    Article  ADS  Google Scholar 

  5. McGaugh, S. S., Lelli, F. & Schombert, J. M. Radial acceleration relation in rotationally supported galaxies. Phys. Rev. Lett. 117, 201101 (2016).

    Article  ADS  Google Scholar 

  6. Randriamampandry, T. H. & Carignan, C. Galaxy mass models: MOND versus dark matter haloes. Mon. Not. R. Astron. Soc. 439, 2132–2145 (2014).

    Article  ADS  Google Scholar 

  7. Rodrigues, D. C., Marra, V., Del Popolo, A. & Davari, Z. Reply to ‘Presence of a fundamental acceleration scale in galaxies’ and ‘A common Milgromiana cceleration scale in nature’. Nat. Astron. 2, 927–929 (2018).

    Article  ADS  Google Scholar 

  8. Chang, Z. & Zhou, Y. Is there a fundamental acceleration scale in galaxies? Mon. Not. R. Astron. Soc. 486, 1658–1666 (2019).

    Article  ADS  Google Scholar 

  9. Li, P., Lelli, F., McGaugh, S. & Schombert, J. Fitting the radial acceleration relation to individual SPARC galaxies. Astron. Astrophys. 615, A3 (2018).

    Article  ADS  Google Scholar 

  10. Feeney, S. M., Mortlock, D. J. & Dalmasso, N. Clarifying the Hubble constant tension with a Bayesian hierarchical model of the local distance ladder. Mon. Not. R. Astron. Soc. 476, 3861–3882 (2018).

    Article  ADS  Google Scholar 

  11. Riess, A. G., Casertano, S., Yuan, W., Macri, L. M. & Scolnic, D. Large Magellanic Cloud Cepheid standards provide a 1% foundation for the determination of the Hubble constant and stronger evidence for physics beyond ΛCDM. Astrophys. J. 876, 85 (2019).

    Article  ADS  Google Scholar 

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Acknowledgements

D.C.R. and V.M. thank CNPq (Brazil) and FAPES (Brazil) for partial financial support. Z.D. thanks the Iran Science Elites Federation for financial support.

Author information

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 Astronomy, Russian Academy of Sciences, Moscow, Russia

    Antonino Del Popolo

  5. INFN sezione di Catania, Catania, Italy

    Antonino Del Popolo

  6. Department of Physics, Sharif University of Technology, Tehran, Iran

    Zahra Davari

Authors
  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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Contributions

D.C.R. and V.M. proposed the first draft and all of the authors contributed to the writing of the manuscript.

Corresponding author

Correspondence to Davi C. Rodrigues.

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Competing interests

The authors declare no competing interests.

Additional information

Peer review information Nature Astronomy thanks Johannes Buchner, Roberto Trotta and the other, anonymous, reviewer(s) for their contribution to the peer review of this work.

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Rodrigues, D.C., Marra, V., Del Popolo, A. et al. Reply to: Overconfidence in Bayesian analyses of galaxy rotation curves. Nat Astron 4, 134–135 (2020). https://doi.org/10.1038/s41550-019-0999-1

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