• [1]

    F. Zwicky, Helvetica Physica Acta 6, 110 (1933)

  • [2]

    S. Smith, Astrophys. J. 83, 23 (1936)

  • [3]

    V. C. Rubin et al., Astrophys. J. 159, 379 (1970)

  • [4]

    V. C. Rubin et al., Astrophys. J. 238, 471 (1980)

  • [5]

    V. C. Rubin, Scientific American 248, 96 (1983)

  • [6]

    D. Clowe et al., Nucl. Phys. B: Proc. Suppl. 173, 28 (2007)

  • [7]

    P. A. R. Ade et al., Astron. Astrophys. 594, A13 (2016)

  • [8]

    O. Adriani et al., Nature 458, 607 (2009)

  • [9]

    X.-Y. Cui, et al. (PandaX-Ⅱ Collaboration), Phys. Rev. Lett. 119, 181302 (2017)

  • [10]

    M. Milgrom, Astrophys. J. 270, 365 (1983)

  • [11]

    M. Milgrom, Astrophys. J. 270, 371 (1983)

  • [12]

    M. Milgrom, Astrophys. J. 270, 384 (1983)

  • [13]

    M. Carmeli, Int. J. Theor. Phys 37, 2621 (1998)

  • [14]

    J. W. Moffat, J. Cosmol. Astropart. Phys. 05, 003 (2005)

  • [15]

    D. Grumiller, Phys. Rev. Lett. 105, 211303 (2010)

  • [16]

    B. Famaey and S. S. McGaugh, Living Rev. Relativ. 15, 10 (2012)

  • [17]

    R. H. Sanders, and S. S. McGaugh, Ann. Rev. Astron. Astrophys. 40, 263 (2002)

  • [18]

    S. M. Kent, Astron. J. 93, 816 (1987)

  • [19]

    K. G. Begeman et al., Mon. Not. Roy. Astron. Soc. 249, 523 (1991)

  • [20]

    B. Famaey and J. Binney, Mon. Not. Roy. Astron. Soc. 363, 603 (2005)

  • [21]

    G. Gentile et al., Mon. Not. Roy. Astron. Soc. 375, 199 (2007)

  • [22]

    R. H. Sanders and E. Noordermeer, Mon. Not. Roy. Astron. Soc. 379, 702 (2007)

  • [23]

    O. Tiret and F. Combes, Astron. Astrophys. 464, 517 (2007)

  • [24]

    S. S. McGaugh, Astrophys. J. 683, 137 (2008)

  • [25]

    R. A. Swaters et al., Astrophys. J. 718, 380 (2010)

  • [26]

    F. Iocco, M. Pato and G. Bertone, Phys. Rev. D 92, 084046 (2015)

  • [27]

    J. D. Bekenstein, Phys. Rev. D 70, 083509 (2004)

  • [28]

    R. H. Sanders, Mon. Not. Roy. Astron. Soc. 363, 459 (2005)

  • [29]

    L. Blanchet and J. Novak, arXiv: 1105.5815[astro-ph.CO] (2011)

  • [30]

    A. Hees et al., Mon. Not. Roy. Astron. Soc. 455, 449 (2016)

  • [31]

    S. McGaugh, Astron. J. 143, 40 (2012)

  • [32]

    F. Lelli et al., Astron. J. 152, 157 (2016)

  • [33]

    S. S. McGaugh et al., Phys. Rev. Lett. 117, 201101 (2016)

  • [34]

    F. Lelli et al., Astrophys. J. 836, 152 (2017)

  • [35]

    P.-F. Li et al., Astron. Astrophys. 615, A3 (2018)

  • [36]

    G. Amir et al., Mon. Not. Roy. Astron. Soc. 487, 2148 (2019)

  • [37]

    D.C. Rodrigues et al., Nat. Astron. 2, 668 (2018)

  • [38]

    Z. Chang and Y. Zhou, Mon. Not. Roy. Astron. Soc. 486, 1658 (2019)

  • [39]

    R. B. Tully et al., Astron. & Astrophys. 54, 661 (1977)

  • [40]

    M. Milgrom, Phys. Rev. D 100, 084039 (2019)

  • [41]

    I. Antoniou and L. Perivolaropoulos, J. Cosmol. Astropart. Phys. 12, 012 (2010)

  • [42]

    J. A. King et al., Mon. Not. Roy. Astron. Soc. 422, 3370 (2012)

  • [43]

    P. A. R. Ade et al., Astron. Astrophys. 571, A23 (2014)

  • [44]

    P. A. R. Ade et al., Astron. Astrophys. 594, A16 (2016)

  • [45]

    Y. Zhou et al., Astrophys. J. 847, 86 (2017)

  • [46]

    Z. Chang et al., Chine. Phys. C 42, 115103 (2018)

  • [47]

    H.-S. Zhao and B. Famaey, Astrophys. J. 638, L9 (2006)

  • [48]

    Z. Chang et al., Eur. Phys. J. C 73, 2447 (2013)

  • [49]

    P. T. Boggs, R. H. Byrd and R. B. Schnabel, SIAM Journal on Scientific and Statistical Computing 8, 1052 (1987)

  • [50]

    P. T. Boggsc et al., Contemporary Mathematics 112, 183 (1990)

  • [51]

    H. Akaike, IEEE Trans. Automatic Control 19, 716 (1974)

  • [52]

    G. Schwarz, Ann. Statist. 6, 461 (1978)

  • [53]

    H. Jeffreys, The theory of probability (Oxford University Press, Oxford U.K.) (1998)

  • [54]

    A. R. Liddle, Mon. Not. Roy. Astron. Soc. 377, L74 (2007)

  • [55]

    H.-N. Lin, X. Li et al., Chine. Phys. C 42, 095101 (2018)

  • [56]

    D. Foreman-Mackey et al., Publications of the Astronomical Society of the Pacific 125, 306 (2013)