Built on

A. G. Riess, S. Casertano, W. Yuan, L. M. Macri, and D. Scolnic, Astrophys. J. 876
Original
1903
Earlier work this paper cites.
V. de Sainte Agathe, C. Balland, H. du Mas des Bourboux, N. G. Busca, M. Blomqvist, J. Guy, J. Rich, A. Font-Ribera, M. M. Pieri, J. E. Bautista, K. Dawson, J. M. Le Goff, A. de la Macorra, N. Palanque-Delabrouille, W. J. Percival, I. Pérez-Ràfols, D. P. Schneider, A. Slosar, and C. Yèche, Astron. Astrophys. 629
Original
1904
Earlier work this paper cites.
K. C. Wong, S. H. Suyu, G. C. F. Chen, C. E. Rusu, M. Millon, D. Sluse, V. Bonvin, C. D. Fassnacht, S. Taubenberger, M. W. Auger, S. Birrer, J. H. H. Chan, F. Courbin, S. Hilbert, O. Tihhonova, T. Treu, A. Agnello, X. Ding, I. Jee, E. Komatsu, A. J. Shajib, A. Sonnenfeld, R. D. Blandford, L. V. E. Koopmans, P. J. Marshall, and G. Meylan, arXiv:1907.04869
Original
1907
Earlier work this paper cites.
E. Di Valentino, A. Melchiorri, E. V. Linder, and J. Silk, Phys. Rev. D 96
Original
1908
Earlier work this paper cites.
W. L. Freedman et al. (HST Collaboration), Astrophys. J. 553
2001
Earlier work this paper cites.
A. Lewis, and S. Bridle, Phys. Rev. D 66
2002
Earlier work this paper cites.
M. J. Reid, J. A. Braatz, J. J. Condon, L. J. Greenhill, C. Henkel, and K. Y. Lo, Astrophys. J. 695
Original
2009
Earlier work this paper cites.

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Original
2011
Cited alongside, same era.
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2012
Cited alongside, same era.
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Cited alongside, same era.
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2015
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Original

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2019

Measuring $H_0$ from low-$z$ datasets

Zhang, Xue, Huang, Qing-Guo

Understand

Adopting the low-redshift observational datasets, including the Pantheon sample of Type Ia supernovae, baryon acoustic oscillation measurements, and the tomographic Alcock-Paczynski method, we determine the Hubble constant to be $67.95^{+0.78}_{-1.03}$ , $69.81^{+2.22}_{-2.70}$ and $66.75^{+3.42}_{-4.23}$ km s$^{-1}$ Mpc$^{-1}$ at 68\% confidence level in the $\Lambda$CDM, $w$CDM and $w_0w_a$CDM models, respectively.

Compared to the Hubble constant given by Riess et al.
in 2019, we conclude that the new physics beyond the standard $\Lambda$CDM model is needed if all of these datasets are reliable.