Cited by 2,590Cosmology and Gravitation TheoriesGalaxies: Formation, Evolution, PhenomenaStellar, planetary, and galactic studies

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The 6dF Galaxy Survey: baryon acoustic oscillations and the local Hubble constant: 6dFGS: BAOs and the local Hubble constant

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Beutler, Florian, Blake, Chris, Colless, Matthew, Jones, D. Heath, Staveley-Smith, Lister, Campbell, Lachlan, Parker, Quentin, Saunders, Will, Watson, Fred·2011·Monthly Notices of the Royal Astronomical Society

DOI 10.1111/j.1365-2966.2011.19250.x

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Abstract

We analyse the large-scale correlation function of the 6dF Galaxy Survey (6dFGS) and detect a baryon acoustic oscillation (BAO) signal at 105 h−1 Mpc. The 6dFGS BAO detection allows us to constrain the distance–redshift relation at zeff= 0.106. We achieve a distance measure of DV(zeff) = 457 ± 27 Mpc and a measurement of the distance ratio, rs(zd)/DV(zeff) = 0.336 ± 0.015 (4.5 per cent precision), where rs(zd) is the sound horizon at the drag epoch zd. The low-effective redshift of 6dFGS makes it a competitive and independent alternative to Cepheids and low-z supernovae in constraining the Hubble constant. We find a Hubble constant of H0= 67 ± 3.2 km s−1 Mpc−1 (4.8 per cent precision) that depends only on the Wilkinson Microwave Anisotropy Probe-7 (WMAP-7) calibration of the sound horizon and on the galaxy clustering in 6dFGS. Compared to earlier BAO studies at higher redshift, our analysis is less dependent on other cosmological parameters. The sensitivity to H0 can be used to break the degeneracy between the dark energy equation of state parameter w and H0 in the cosmic microwave background data. We determine that w=−0.97 ± 0.13, using only WMAP-7 and BAO data from both 6dFGS and Percival et al. (2010). We also discuss predictions for the large-scale correlation function of two future wide-angle surveys: the Wide field ASKAP L-band Legacy All-sky Blind surveY (WALLABY) blind H i survey (with the Australian Square Kilometre Array Pathfinder, ASKAP) and the proposed Transforming Astronomical Imaging surveys through Polychromatic Analysis of Nebulae (TAIPAN) all-southern-sky optical galaxy survey with the UK Schmidt Telescope. We find that both surveys are very likely to yield detections of the BAO peak, making WALLABY the first radio galaxy survey to do so. We also predict that TAIPAN has the potential to constrain the Hubble constant with 3 per cent precision.

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SEVEN-YEAR WILKINSON MICROWAVE ANISOTROPY PROBE(WMAP) OBSERVATIONS: COSMOLOGICAL INTERPRETATION
Komatsu, E., Smith, K. M., Dunkley, J., Bennett, C. L., Gold, B., Hinshaw, G., Jarosik, N., Larson, D., Nolta, M. R., Page, L., et al. (2011) · The Astrophysical Journal Supplement Series · doi:10.1088/0067-0049/192/2/18 · Cited by 8,802
The Sloan Digital Sky Survey: Technical Summary
York, D., Adelman, J., Anderson, J., Anderson, S., Annis, J., Bahcall, N., Bakken, J., Barkhouser, R., Bastian, S., Berman, E., et al. (2000) · The Astronomical Journal · doi:10.1086/301513 · Cited by 8,368 · cited 1×
“The Sloan Digital Sky Survey (SDSS; York et al. 2000), and the 2dF Galaxy Redshift Survey (2dFGRS; Colless et al. 2001) were the first redshift surveys which have directly detected the BAO signal.”
Method
FIVE-YEAR WILKINSON MICROWAVE ANISOTROPY PROBE OBSERVATIONS: COSMOLOGICAL INTERPRETATION
Komatsu, E., Dunkley, J., Nolta, M. R., Bennett, C. L., Gold, B., Hinshaw, G., Jarosik, N., Larson, D., Limon, M., Page, L., et al. (2009) · The Astrophysical Journal Supplement Series · doi:10.1088/0067-0049/180/2/330 · Cited by 5,786
THE SEVENTH DATA RELEASE OF THE SLOAN DIGITAL SKY SURVEY
Abazajian, K. N., Adelman-McCarthy, J. K., Agüeros, M. A., Allam, S. S., Prieto, C. A., An, D., Anderson, K. S. J., Anderson, S. F., Annis, J., Bahcall, N. A., et al. (2009) · The Astrophysical Journal Supplement Series · doi:10.1088/0067-0049/182/2/543 · Cited by 5,341 · cited 1×
“The volume of the 6dF Galaxy Survey is approximately as large as the volume covered by the 2dF Galaxy Redshift Survey, with a sample density similar to SDSSDR7 (Abazajian et al. 2009).”
Method
The Design and Implementation of FFTW3
Frigo, M., & Johnson, S. G. (2005) · Proceedings of the IEEE · doi:10.1109/jproc.2004.840301 · Cited by 5,086
Efficient Computation of Cosmic Microwave Background Anisotropies in Closed Friedmann‐Robertson‐Walker Models
Lewis, A., Challinor, A., & Lasenby, A. (2000) · The Astrophysical Journal · doi:10.1086/309179 · Cited by 4,920
Detection of the Baryon Acoustic Peak in the Large‐Scale Correlation Function of SDSS Luminous Red Galaxies
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 4,641 · cited 9×
“We derive the parameter (Eisenstein et al. 2005) A(zeff) = 100DV (zeff) √ Ωmh2 czeff , (27) which has no dependence on the Hubble constant since DV ∝ h−1.”
BackgroundMethodInfluential
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., Robert C. Kennicutt, Jr., Ford, H. C., Graham, J. A., et al. (2001) · The Astrophysical Journal · doi:10.1086/320638 · Cited by 3,543
Clustering in real space and in redshift space
Kaiser, N. (1987) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/227.1.1 · Cited by 2,762 · cited 1×
“The model of linear redshift space distortions introduced by Kaiser (1987) is based on the plane parallel approximation.”
Method
Detection of the Baryon Acoustic Peak in the Large-Scale Correlation Function of SDSS Luminous Red Galaxies
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) · Cited by 2,568

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Research works printed but not linked: 2

Arnalte-Mur, 2011, MNRAS
Sanchez, 2008, MNRAS, 390, 1470

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Neutrino mass bounds from DESI 2024 are relaxed by Planck PR4 and cosmological supernovae
Allali, I. J., & Notari, A. (2024) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2024/12/020 · Cited by 42
“Using the most recent eBOSS DR16 measurements from SDSS [5] (in combination with 6DFGS [25] and older data from SDSS) the bound is substantially weaker: m ν 0 .”
Implications of the cosmic calibration tension beyond H 0 and the synergy between early- and late-time new physics
Poulin, V., Smith, T. L., Calderón, R., & Simon, T. (2025) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.111.083552 · Cited by 52
Redshift drift exploration for interacting dark energy
Geng, J.-J., Li, Y.-H., Zhang, J.-F., & Zhang, X. (2015) · The European Physical Journal C · doi:10.1140/epjc/s10052-015-3581-8 · Cited by 42
(Lack of) Cosmological evidence for dark radiation after Planck
Verde, L., Feeney, S. M., Mortlock, D. J., & Peiris, H. V. (2013) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2013/09/013 · Cited by 42
“While in some cases the priors can be physically motivated, this is not always possible; in the latter case, the Bayesian answer to the model comparison question calculated with specific prior choices cannot be considered definitive.”
Background
Cosmic equation of state from combined angular diameter distances: Does the tension with luminosity distances exist?
Cao, S., & Zhu, Z. (2014) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.90.083006 · Cited by 43
Nonlocal teleparallel cosmology
Bahamonde, S., Capozzıello, S., Faizal, M., & Nunes, R. C. (2017) · The European Physical Journal C · doi:10.1140/epjc/s10052-017-5210-1 · Cited by 42
Measuring growth index in a universe with massive neutrinos: A revisit of the general relativity test with the latest observations
Zhao, M.-M., Zhang, J.-F., & Zhang, X. (2018) · Physics Letters B · doi:10.1016/j.physletb.2018.02.042 · Cited by 44
Probing the sign-changeable interaction between dark energy and dark matter with current observations
Guo, J.-J., Zhang, J.-F., Li, Y.-H., He, D.-Z., & Zhang, X. (2018) · Science China Physics Mechanics and Astronomy · doi:10.1007/s11433-017-9131-9 · Cited by 44
Investigating the Hubble Constant Tension: Two Numbers in the Standard Cosmological Model
Lin, W., Mack, K. J., & Hou, L. (2020) · The Astrophysical Journal Letters · doi:10.3847/2041-8213/abc894 · Cited by 42
“Galaxy BAOs consist of measurements at zeff=0.106 (Beutler et al. 2011), 0.15 (Ross et al. 2015), 0.38, 0.51, 0.61 (Alam et al. 2017), and 1.52 (Ata et al. 2018).”
Influential
Metastable dark energy models in light of Planck 2018 data: Alleviating the H0 tension
Yang, W., Valentino, E. D., Pan, S., Basilakos, S., & Paliathanasis, A. (2020) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.102.063503 · Cited by 43
“[188] F.”
MethodInfluential
Dynamical dark sectors and neutrino masses and abundances
Yang, W., Valentino, E. D., Mena, O., & Pan, S. (2020) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.102.023535 · Cited by 42
“• Baryon Acoustic Oscillations (BAO): we make use of several BAO measurements from different cosmological observations, as considered by the Planck collaboration [67]: 6dFGS [70], SDSSMGS [71], and BOSS DR12 [72] surveys.”
Method
Reconstruction of the neutrino mass as a function of redshift
Lorenz, C. S., Funcke, L., Löffler, M., & Calabrese, E. (2021) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.104.123518 · Cited by 42
“) BAO: We use BAO from 6dF [127], the Sloan Digital Sky Survey (SDSS) DR7 Main Galaxy Sample (MGS) [128] and the SDSS Baryon Oscillation Spectroscopic Survey (BOSS) twelfth data release (DR12) [129].”
Thermal WIMPs and the scale of new physics
Athron, P., Kozar, N., Balazs, C., Beniwal, A., Bloor, S., Bringmann, T., Brod, J., Chang, C., Cornell, J. M., Farmer, B., et al. (2021) · The European Physical Journal C · doi:10.1140/epjc/s10052-021-09712-6 · Cited by 41
Multi-interacting dark energy and its cosmological implications
Lucca, M. (2021) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.104.083510 · Cited by 46
“In particular, we adopt the same baseline combination of probes which relies on data from Planck 2018 [2] (temperature, polarization and lensing likelihoods), the 6dF Galaxy Survey (6dFGS) [52], the Sloan Digital Sky Survey (SDSS), the Baryon Oscillation Spectroscopic Survey (BOSS) [53, 54] and the SNIa Pantheon catal…”
Method
Viscous cosmology in the Weyl-type f(Q, T) gravity
Gadbail, G. N., Arora, S., & Sahoo, P. K. (2021) · The European Physical Journal C · doi:10.1140/epjc/s10052-021-09889-w · Cited by 42
SIMULTANEOUS CONSTRAINTS ON THE NUMBER AND MASS OF RELATIVISTIC SPECIES
Riemer–Sørensen, S., Parkinson, D., Davis, T. M., & Blake, C. (2013) · The Astrophysical Journal · doi:10.1088/0004-637x/763/2/89 · Cited by 41
“BAO: The BAO scale measured at z = 0.106 (rs/DV = 0.336 ± 0.015) from the Six Degree Field Galaxy Survey (6dFGS) (Beutler et al. 2011), the reconstructed value at z = 0.35 (rs/DV = 0.1126 ± 0.0022) from Sloan Digital Sky Survey (SDSS) Luminous Red Galaxies (LRG) (Padmanabhan et al. 2012), and z =…”
MethodInfluentialSelf-citation
Return of Harrison–Zeldovich spectrum in light of recent cosmological tensions
Jiang, J.-Q., Ye, G., & Yun-song Piao, A. (2023) · Monthly Notices of the Royal Astronomical Society Letters · doi:10.1093/mnrasl/slad137 · Cited by 43
Prospects for Probing the Interaction between Dark Energy and Dark Matter Using Gravitational-wave Dark Sirens with Neutron Star Tidal Deformation
Li, T.-N., Jin, S.-J., Li, H., Zhang, J., & Zhang, X. (2024) · The Astrophysical Journal · doi:10.3847/1538-4357/ad1bc9 · Cited by 47
Cosmology with varying fundamental constants from hyperlight, coupled scalars
Baryakhtar, M., Simon, O., & Weiner, Z. J. (2024) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.110.083505 · Cited by 42
Quintessence with Yukawa interaction
Costa, A. A., Olivari, L. C., & Elcio Abdalla, A. (2015) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.92.103501 · Cited by 41
Distance priors from Planck 2015 data
Huang, Q.-G., Wang, K., & Wang, S. (2015) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2015/12/022 · Cited by 41
Measuring baryon acoustic oscillations from the clustering of voids
Liang, Y., Zhao, C., Chuang, C.-H., Kitaura, F.-S., & TAO, C. (2016) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stw884 · Cited by 41
“The BAO signal has been improved by further SDSS measurements and other galaxy redshift surveys (Eisenstein et al. 2005b; Percival et al. 2010; Blake et al. 2011; Beutler et al. 2011; ?”
Method
Measuring the 2D baryon acoustic oscillation signal of galaxies in WiggleZ: cosmological constraints
Hinton, S. R., Kazin, E. A., Davis, T. M., Blake, C., Brough, S., Colless, M., Couch, W. J., Drinkwater, M. J., Glazebrook, K., Jurek, R. J., et al. (2016) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stw2725 · Cited by 41
“We model the BAO peak smoothing caused by displacement of matter due to bulk flows with a smoothing parameter (Crocce & Scoccimarro 2008; Sánchez et al. 2008, 2009; Blake et al. 2011b; Beutler et al. 2011).”
MethodSelf-citation
Constraints on the sum of neutrino masses using cosmological data including the latest extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample
Wang, S., Wang, Y., & Xia, D. (2018) · Chinese Physics C · doi:10.1088/1674-1137/42/6/065103 · Cited by 41
The BINGO telescope: a new instrument exploring the new 21 cm cosmology window
Wuensche, C. A. (2019) · Journal of Physics Conference Series · doi:10.1088/1742-6596/1269/1/012002 · Cited by 41
Observational constraints on cosmological models with Chaplygin gas and quadratic equation of state
Sharov, G. S. (2016) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2016/06/023 · Cited by 41
“[25] [9, 24] [10] [32] [33] [22] [29] [18] [21] [27, 28, 31] [26] rs(zd) 147.”
Axi-Higgs cosmology
Fung, L. W. H., Li, L., Liu, T., Luu, H. N., Qiu, Y.-C., & Tye, S.-H. H. (2021) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2021/08/057 · Cited by 41
“Also, Hart & Chluba used a combined set of only low-z BAO data: 6dF [57] + MGS [58] + BOSS DR12 [65], which leads to a different constraint on rdh compared to Eq.”
Method
Cosmology beyond BAO from the 3D distribution of the Lyman-α forest
Cuceu, A., Font-Ribera, A., Joachimi, B., & Nadathur, S. (2021) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stab1999 · Cited by 41
Using dark energy to suppress power at small scales
Kunz, M., Nesseris, S., & Sawicki, I. (2015) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.92.063006 · Cited by 41
Revisiting CMB constraints on dark matter annihilation
Kawasaki, M., Nakatsuka, H., Nakayama, K., & Sekiguchi, T. (2021) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2021/12/015 · Cited by 40
An axially symmetric transitioning models with observational constraints
Bhardwaj, V. K., Dixit, A., Rani, R., Goswami, G. K., & Pradhan, A. (2022) · Chinese Journal of Physics · doi:10.1016/j.cjph.2022.09.007 · Cited by 40
Massive neutrino self-interactions and inflation
Choudhury, S. R., Hannestad, S., & Tram, T. (2022) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2022/10/018 · Cited by 40
“In addition to the CMB power spectra, we use an additional dataset combination which consists of Planck 2018 CMB lensing [50], BAO and RSD measurements from SDSS-III BOSS DR12 [51], additional BAO measurements from MGS [52] and 6dFGS [53], and SNe Ia luminosity distance measurements from the Pantheon sample [54].”
Method
Cosmological constraint precision of photometric and spectroscopic multi-probe surveys of China Space Station Telescope ( CSST )
Miao, H., Gong, Y., Chen, X., Huang, Z., Li, X.-D., & Zhan, H. (2022) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stac3583 · Cited by 40
“Based on a variety of observations in the past two decades (Percival et al. 2010; Eisenstein et al. 2011; Komatsu et al. 2011; Beutler et al. 2011; Sievers et al. 2013; Hinshaw et al. 2013; Hou et al. 2014; Planck Collaboration et al. 2014),we have entered the era of precision cosmology, and…”
Background
Cosmological tests of parametrization q = α − β H in f(Q) FLRW cosmology
Bouali, A., Shukla, B. K., Chaudhary, H., Tiwari, R. K., Samar, M., & Mustafa, G. (2023) · International Journal of Geometric Methods in Modern Physics · doi:10.1142/s0219887823501529 · Cited by 40
Cosmic evolution in f ( Q , T ) gravity: Exploring a higher-order time-dependent function of deceleration parameter with observational constraints
Khurana, M., Chaudhary, H., Mumtaz, S., Pacif, S. K. J., & Mustafa, G. (2023) · Physics of the Dark Universe · doi:10.1016/j.dark.2023.101408 · Cited by 40
Cosmological constraints from the cross-correlation of DESI Luminous Red Galaxies with CMB lensing from Planck PR4 and ACT DR6
Sailer, N., Kim, J., Ferraro, S., Madhavacheril, M. S., White, M. J., Abril-Cabezas, I., Aguilar, J., Ahlen, S. P., Bond, J. R., Brooks, D., et al. (2025) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2025/06/008 · Cited by 40
Parametrized modified gravity constraints after Planck
Hu, B., Liguori, M., Bartolo, N., & Matarrese, S. (2013) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.88.123514 · Cited by 38
Interacting viscous dark fluids
Avelino, A., Leyva, Y., & Ureña-López, L. (2013) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.88.123004 · Cited by 33
Implications of the B -mode polarization measurement for direct detection of inflationary gravitational waves
Kuroyanagi, S., Tsujikawa, S., Chiba, T., & Sugiyama, N. (2014) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.90.063513 · Cited by 40
Growth of matter perturbations in clustered holographic dark energy cosmologies
Mehrabi, A., Basilakos, S., Malekjani, M., & Davari, Z. (2015) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.92.123513 · Cited by 41
The galaxy–halo connection in the VIDEO survey at 0.5 <z< 1.7
Hatfield, P., Lindsay, S., Jarvis, M. J., Häußler, B., Vaccari, M., & Verma, A. (2016) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stw769 · Cited by 40
“Therefore, when fitting the correlation functions, we treat the constraint as part of the model and fit data to the theoretical observed function, as in Beutler et al. (2011).”
Method
Unbiased pseudo-Cℓpower spectrum estimation with mode projection
Elsner, F., Leistedt, B., & Peiris, H. V. (2016) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stw2752 · Cited by 40
“…et al. (1996); Norberg et al. (2001); Blake & Wall (2002); Zehavi et al. (2002); Tegmark et al. (2004); Croom et al. (2005); Eisenstein et al. (2005); Coil et al. (2008); Reid et al. (2010); Beutler et al. (2011); Kim et al. (2014); Crocce et al. (2016) for constraints on galaxy clustering.”
AGNs and Their Host Galaxies in the Local Universe: Two Mass-independent Eddington Ratio Distribution Functions Characterize Black Hole Growth
Weigel, A. K., Schawinski, K., Čaplar, N., Wong, O. I., Treister, E., & Trakhtenbrot, B. (2017) · The Astrophysical Journal · doi:10.3847/1538-4357/aa803b · Cited by 44
“Photometric and spectroscopic redshifts for EMU will be provided by SkyMapper (Keller et al. 2007), WALLABY (Koribalski 2012) and TAIPAN (Beutler et al. 2011).”
Method
Model-independent constraints on Lorentz invariance violation via the cosmographic approach
Zou, X.-B., Deng, H.-K., Yin, Z.-Y., & Wei, H. (2017) · Physics Letters B · doi:10.1016/j.physletb.2017.11.053 · Cited by 40
Measurement of Hubble constant with stellar-mass binary black holes
Nishizawa, A. (2017) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.96.101303 · Cited by 40
Power spectrum multipoles on the curved sky: an application to the 6-degree Field Galaxy Survey
Blake, C., Carter, P., & Koda, J. (2018) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/sty1814 · Cited by 40
Self-citation

Authors: Beutler, F., Blake, C., Colless, M., Jones, D. H., Staveley-Smith, L., Campbell, L., Parker, Q., Saunders, W., & Watson, F.
Affiliations: The University of Western Australia (AU)
Swinburne University of Technology (AU)
Australian Astronomical Observatory (AU)
Monash University (AU)
Western Kentucky University (US)
Corresponding author: Beutler, Florian
ORCID: Beutler, Florian
Blake, Chris
Colless, Matthew
Jones, D. Heath
Campbell, Lachlan
Parker, Quentin
Watson, Fred
Venue: Monthly Notices of the Royal Astronomical Society
Publisher: Oxford University Press (OUP)
Published: 2011-07-25
Volume: 416
Issue: 4
Pages: 3017-3032
ISSN: 0035-8711 (ISSN-L)
DOI: 10.1111/j.1365-2966.2011.19250.x
OpenAlex: W2121951791
Cited by: 2,590
References: 87
Citations by year: 2026: 90 · 2025: 191 · 2024: 228 · 2023: 207 · 2022: 210 · 2021: 236 · 2020: 241 · 2019: 207 · 2018: 176 · 2017: 178 · 2016: 167 · 2015: 131 · 2014: 147 · 2013: 113 · 2012: 61
FWCI: 54.71
Type: journal article
Language: en
Open access: bronze
doi.org
Locations: Monthly Notices of the Royal Astronomical Society (publishedVersion)
UWA Profiles and Research Repository (UWA) (publishedVersion, other-oa)
arXiv (Cornell University) (submittedVersion)
Figshare (submittedVersion, cc-by)
The HKU Scholars Hub (University of Hong Kong) (submittedVersion)
ANU Open Research (Australian National University) (submittedVersion)
Swinburne figshare (Swinburne University of Technology) (submittedVersion)
arXiv (Cornell University)
American Astronomical Society Meeting Abstracts #219
Swinburne figshare (Swinburne University of Technology)
Funders: Australian Government
Australian National University
Australian Research Council (DP0208876)
Topics: Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Cosmology and Gravitation Theories
Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Galaxies: Formation, Evolution, Phenomena
Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Stellar, planetary, and galactic studies
Keywords: baryon acoustic oscillations, 6dF Galaxy Survey, local Hubble constant, sound horizon, distance-redshift relation, dark energy equation of state, wallabies, taipan, radio galaxy surveys, cosmological constraints

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The 6dF Galaxy Survey: baryon acoustic oscillations and the local Hubble constant: 6dFGS: BAOs and the local Hubble constant

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