The DOI matches its Crossref record; 27 of the 27 references it cites were found in a registry or an index.
THE 1% CONCORDANCE HUBBLE CONSTANT
Open accessAbstract
The determination of the Hubble constant has been a central goal in observational astrophysics for nearly a hundred years. Extraordinary progress has occurred in recent years on two fronts: the cosmic distance ladder measurements at low redshift and cosmic microwave background (CMB) measurements at high redshift. The CMB is used to predict the current expansion rate through a best-fit cosmological model. Complementary progress has been made with baryon acoustic oscillation (BAO) measurements at relatively low redshifts. While BAO data do not independently determine a Hubble constant, they are important for constraints on possible solutions and checks on cosmic consistency. A precise determination of the Hubble constant is of great value, but it is more important to compare the high and low redshift measurements to test our cosmological model. Significant tension would suggest either uncertainties not accounted for in the experimental estimates or the discovery of new physics beyond the standard model of cosmology. In this paper we examine in detail the tension between the CMB, BAO, and cosmic distance ladder data sets. We find that these measurements are consistent within reasonable statistical expectations and we combine them to determine a best-fit Hubble constant of 69.6 ± 0.7 km s −1 Mpc −1 . This value is based upon WMAP 9+SPT+ACT+6dFGS+BOSS/DR11+ H 0 /Riess; we explore alternate data combinations in the text. The combined data constrain the Hubble constant to 1%, with no compelling evidence for new physics.
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NINE-YEAR WILKINSON MICROWAVE ANISOTROPY PROBE ( WMAP ) OBSERVATIONS: COSMOLOGICAL PARAMETER RESULTS
Hinshaw, G., Larson, D., Komatsu, E., Spergel, D. N., Bennett, C. L., Dunkley, J., Nolta, M. R., Halpern, M., Hill, R. S., Odegard, N., et al. (2013) · The Astrophysical Journal Supplement Series · doi:10.1088/0067-0049/208/2/19 · Cited by 5,121
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Eisenstein, D. J., Zehavi, I., Hogg, D. W., Scoccimarro, R., Blanton, M. R., Nichol, R. C., Scranton, R., Seo, H., Tegmark, M., Zheng, Z., et al. (2005) · The Astrophysical Journal · doi:10.1086/466512 · Cited by 4,629
Final Results from the Hubble Space Telescope Key Project to Measure the Hubble Constant
Freedman, W. L., Madore, B. F., Gibson, B. K., Ferrarese, L., Kelson, D. D., Sakai, S., Mould, J. R., Kennicutt, Jr., Ford, H. C., Graham, J. A., et al. (2001) · The Astrophysical Journal · doi:10.1086/320638 · Cited by 3,298
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A relation between distance and radial velocity among extra-galactic nebulae
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NINE-YEAR WILKINSON MICROWAVE ANISOTROPY PROBE ( WMAP ) OBSERVATIONS: FINAL MAPS AND RESULTS
Bennett, C. L., Larson, D., Weiland, J. L., Jarosik, N., Hinshaw, G., Odegard, N., Smith, K. M., Hill, R. S., Gold, B., Halpern, M., et al. (2013) · The Astrophysical Journal Supplement Series · doi:10.1088/0067-0049/208/2/20 · Cited by 2,408
Self-citationBaryonic Features in the Matter Transfer Function
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Cited by
Alam, S., Ata, M., Bailey, S., Beutler, F., Bizyaev, D., Blazek, J. A., Bolton, A. S., Brownstein, J. R., Burden, A., Chuang, C.-H., et al. (2017) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stx721 · Cited by 3,056
Quantifying discordance in the 2015 Planck CMB spectrum
Addison, G. E., Huang, Y., Watts, D. J., Bennett, C. L., Halpern, M., Hinshaw, G., & Weiland, J. L. (2016) · The Astrophysical Journal · doi:10.3847/0004-637x/818/2/132 · Cited by 235
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Metadata
- Authors
- Bennett, C. L., Larson, D., Weiland, J. L., & Hinshaw, G.
- Venue
- The Astrophysical Journal
- Publisher
- American Astronomical Society
- Published
- 2014-10-01
- Volume
- 794
- Issue
- 2
- Pages
- 135
- ISSN
- 0004-637X (ISSN-L)
- 1538-4357
- OpenAlex
- W2166156153
- Cited by
- 432
- References
- 27
- FWCI
- 14.73
- Type
- journal article
- Language
- en
- Open access
- bronze
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