• [1]

    A. G. Riess et al., Astron. J. 116, 1009 (1998), arXiv:astro-ph/9805201

  • [2]

    S. Perlmutter et al., Astrophys. J. 517, 565 (1999), arXiv:astro-ph/9812133

  • [3]

    G. W. Horndeski, Int. J. Theor. Phys. 10, 363 (1974)

  • [4]

    C. Deffayet, X. Gao, D. A. Steer et al., Phys. Rev. D 84, 064039 (2011), arXiv:1103.3260[hep-th

  • [5]

    T. Kobayashi, M. Yamaguchi, and J. Yokoyama, Prog. Theor. Phys. 126, 511 (2011), arXiv:1105.5723[hep-th

  • [6]

    L. Heisenberg, JCAP 1405, 015 (2014), arXiv:1402.7026[hep-th

  • [7]

    A. De Felice, L. Heisenberg, R. Kase et al., JCAP 1606(06), 048 (2016), arXiv:1603.05806[gr-qc

  • [8]

    C. de Rham, G. Gabadadze, and A. J. Tolley, Phys. Rev. Lett. 106, 231101 (2011), arXiv:1011.1232[hep-th

  • [9]

    C. de Rham and G. Gabadadze, Phys. Rev. D 82, 044020 (2010), arXiv:1007.0443[hep-th

  • [10]

    B. P. Abbott et al., Phys. Rev. Lett. 116(6), 061102 (2016), arXiv:1602.03837[gr-qc

  • [11]

    B. P. Abbott et al., Phys. Rev. Lett. 119(16), 161101 (2017), arXiv:1710.05832[gr-qc

  • [12]

    T. Baker, E. Bellini, P. G. Ferreira et al., Phys. Rev. Lett. 119(25), 251301 (2017), arXiv:1710.06394[astro-ph.CO

  • [13]

    J. Sakstein and B. Jain, Phys. Rev. Lett. 119(25), 251303 (2017), arXiv:1710.05893[astro-ph.CO

  • [14]

    P. A. R. Ade et al., Astron. Astrophys. 594, A13 (2016), arXiv:1502.01589[astro-ph.CO

  • [15]

    A. G. Riess, S. Casertano, W. Yuan et al., Astrophys. J. 876(1), 85 (2019), arXiv:1903.07603[astroph.CO

  • [16]

    K. C. Wong et al., Mon. Not. Roy. Astron. Soc. 498(1), 1420-1439 (2020), arXiv:1907.04869 [astro-ph.CO

  • [17]

    G. C.-F. Chen et al., Mon. Not. Roy. Astron. Soc. 490(2), 1743-1773 (2019), arXiv:1907.02533 [astro-ph.CO

  • [18]

    W. L. Freedman et al., The Carnegie-Chicago Hubble Program. VIII. An Independent Determination of the Hubble Constant Based on the Tip of the Red Giant Branch, arXiv:1907.05922 [astro-ph.CO]

  • [19]

    W. Yuan, A. G. Riess, L. M. Macri et al., Astrophys. J. 886, 61 (2019), arXiv:1908.00993[astroph.GA

  • [20]

    J. Renk, M. Zumalacrregui, F. Montanari et al., JCAP 1710(10), 020 (2017), arXiv:1707.02263[astro-ph.CO

  • [21]

    R. C. Nunes, JCAP 1805(05), 052 (2018), arXiv:1802.02281[gr-qc

  • [22]

    H. Desmond, B. Jain, and J. Sakstein, Phys. Rev. D 100(4), 043537 (2019), arXiv:1907.03778 [astro-ph.CO

  • [23]

    U. Alam, S. Bag, and V. Sahni, Phys. Rev. D 95(2), 023524 (2017), arXiv:1605.04707[astro-ph.CO

  • [24]

    N. Khosravi, S. Baghram, N. Afshordi et al., Phys. Rev. D 99(10), 103526 (2019), arXiv:1710.09366[astro-ph.CO

  • [25]

    E. Di Valentino, E. V. Linder, and A. Melchiorri, Phys. Rev. D 97(4), 043528 (2018), arXiv:1710.02153[astro-ph.CO

  • [26]

    A. Banihashemi, N. Khosravi, and A. H. Shirazi, Phys. Rev. D 99(8), 083509 (2019), arXiv:1810.11007[astro-ph.CO

  • [27]

    V. Poulin, T. L. Smith, T. Karwal et al., Phys. Rev. Lett. 122(22), 221301 (2019), arXiv:1811.04083[astro-ph.CO

  • [28]

    K. Vattis, S. M. Koushiappas, and A. Loeb, Phys. Rev. D 99(12), 121302 (2019), arXiv:1903.06220[astro-ph.CO

  • [29]

    S. Kumar, R. C. Nunes, and S. K. Yadav, Eur. Phys. J. C 79(7), 576 (2019), arXiv:1903.04865[astro-ph.CO

  • [30]

    W. Yang, S. Pan, E. Di Valentino et al., JCAP 1809(09), 019 (2018), arXiv:1805.08252[astro-ph.CO

  • [31]

    C. D. Kreisch, F. Y. Cyr-Racine, and O. Dor, Phys. Rev. D 101(12), 123505 (2020), arXiv:1902.00534 [astro-ph.CO

  • [32]

    X. Li and A. Shafieloo, Astrophys. J. Lett. 883(1), L3 (2019), arXiv:1906.08275 [astro-ph.CO

  • [33]

    K. Dutta, Ruchika, A. Roy et al., Gen. Rel. Grav. 52(2), 15 (2020), arXiv:1808.06623 [astro-ph.CO

  • [34]

    L. Visinelli, S. Vagnozzi, and U. Danielsson, Symmetry 11, 1035 (2019), arXiv:1907.07953[astro-ph.CO

  • [35]

    S. Panpanich and P. Burikham, Phys. Rev. D 98(6), 064008 (2018), arXiv:1806.06271[gr-qc

  • [36]

    Z. K. Guo, Y. S. Piao, X. M. Zhang et al., Phys. Lett. B 608, 177 (2005), arXiv:astro-ph/0410654

  • [37]

    E. Elizalde, S. Nojiri, and S. D. Odintsov, Phys. Rev. D 70, 043539 (2004), arXiv:hep-th/0405034

  • [38]

    E. Elizalde, S. Nojiri, S. D. Odintsov et al., Phys. Rev. D 77, 106005 (2008), arXiv:0803.1311[hepth

  • [39]

    S. Alexander and E. McDonough, Physics Letters B, 797 (2019), arXiv:1904.08912[astro-ph.CO

  • [40]

    E. Colgin and H. Yavartanoo, Phys. Lett. B 797, 134907 (2019), arXiv:1905.02555 [astroph.CO

  • [41]

    A. Naruko, D. Yoshida, and S. Mukohyama, Class. Quant. Grav. 33(9), 09LT01 (2016), arXiv:1512.06977[gr-qc

  • [42]

    E. N. Saridakis and M. Tsoukalas, Phys. Rev. D 93(12), 124032 (2016), arXiv:1601.06734[gr-qc

  • [43]

    N. Aghanim et al. [Planck Collaboration], Astron. Astrophys. 641, A6 (2020), arXiv:1807.06209 [astro-ph.CO

  • [44]

    L. Amendola, Phys. Rev. D 62, 043511 (2000), arXiv:astro-ph/9908023

  • [45]

    S. Tsujikawa, arXiv:1004.1493 [astro-ph.CO]

  • [46]

    K. Hinterbichler, J. Khoury, A. Levy et al., Phys. Rev. D 84, 103521 (2011), arXiv:1107.2112[astro-ph.CO

  • [47]

    J. Khoury and A. Weltman, Phys. Rev. Lett. 93, 171104 (2004), arXiv:astro-ph/0309300

  • [48]

    J. Khoury and A. Weltman, Phys. Rev. D 69, 044026 (2004), arXiv:astroph/0309411

  • [49]

    H. Yu, B. Ratra and F. Wang, Astrophys. J. 856(1), 3 (2018), arXiv:1711.03437[astro-ph.CO

  • [50]

    D. M. Scolnic et al., Astrophys. J. 859(2), 101 (2018), arXiv:1710.00845[astroph.CO

  • [51]

    D. Jones, D. Scolnic, A. Riess et al., Astrophys. J. 857(1), 51 (2018), arXiv:1710.00846[astro-ph.CO

  • [52]

    A. Conley et al., Astrophys. J. Suppl. 192, 1 (2011), arXiv:1104.1443[astro-ph.CO

  • [53]

    D. Richardson, R. L. Jenkins, J. Wright et al., Astron. J. 147, 118 (2014), arXiv:1403.5755[astro-ph.SR

  • [54]

    W. Hu and N. Sugiyama, Astrophys. J. 471, 542 (1996), arXiv:astro-ph/9510117

  • [55]

    D. J. Eisenstein and W. Hu, Astrophys. J. 496, 605 (1998), arXiv:astro-ph/9709112

  • [56]

    P. A. R. Ade et al., Astron. Astrophys. 571, A16 (2014), arXiv:1303.5076[astro-ph.CO

  • [57]

    W. J. Percival, S. Cole, D. J. Eisenstein et al., Mon. Not. Roy. Astron. Soc. 381, 1053 (2007), arXiv:0705.3323[astro-ph

  • [58]

    F. Beutler, C. Blake, M. Colless et al., Mon. Not. Roy. Astron. Soc. 416, 3017 (2011)

  • [59]

    A. J. Ross, L. Samushia, C. Howlett et al., Mon. Not. Roy. Astron. Soc. 449(1), 835 (2015), arXiv:1409.3242[astro-ph.CO

  • [60]

    S. Alam et al., Mon. Not. Roy. Astron. Soc. 470(3), 2617 (2017), arXiv:1607.03155[astroph.CO

  • [61]

    F. Arevalo, A. Cid, and J. Moya, Eur. Phys. J. C 77(8), 565 (2017), arXiv:1610.09330[astro-ph.CO

  • [62]

    W. Hu, M. Fukugita, M. Zaldarriaga et al., Astrophys. J. 549, 669 (2001), arXiv:astro-ph/0006436[astro-ph

  • [63]

    M. Doran and M. Lilley, Mon. Not. Roy. Astron. Soc. 330, 965-970 (2002), arXiv:astro-ph/0104486[astro-ph

  • [64]

    N. Aghanim et al., Astron. Astrophys. 594, A11 (2016), arXiv:1507.02704[astro-ph.CO