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The 6dF Galaxy Survey: baryon acoustic oscillations and the local Hubble constant: 6dFGS: BAOs and the local Hubble constant
Open accessAbstract
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.”
MethodFIVE-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).”
MethodThe 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
Lewis, A., Challinor, A., & Lasenby, A. (2000) · The Astrophysical Journal · doi:10.1086/309179 · Cited by 4,920
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.”
BackgroundMethodInfluentialFinal 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.”
MethodEisenstein, 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
Research works printed but not linked: 2
- Arnalte-Mur, 2011, MNRAS
- Sanchez, 2008, MNRAS, 390, 1470
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Items 101–200 of 1,006
Joudaki, S., Blake, C., Johnson, A., Amon, A., Asgari, M., Choi, A., Erben, T., Glazebrook, K., Harnois-Déraps, J., Heymans, C., et al. (2018) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stx2820 · Cited by 291
“…deviations from GR with the Canada-France-Hawaii Telescope Lensing Survey (CFHTLenS; Heymans et al. 2012; Hildebrandt et al. 2012; Erben et al. 2013; Miller et al. 2013), WiggleZ Dark Energy Survey (Blake et al. 2011, 2012), and the 6-degree-Field Galaxy Survey (6dFGS; Beutler et al. 2011, 2012).”
BackgroundSelf-citationGil-Marín, H., Bautista, J., Paviot, R., Vargas-Magaña, M., de la Torre, S., Fromenteau, S., Alam, S., Avila, S., Burtin, E., Chuang, C.-H., et al. (2020) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/staa2455 · Cited by 287
“…a plethora of measurements has been performed on spectroscopic galaxy surveys at different epochs: 6-degree Field Survey (6dF; Jones et al. 2009; Beutler et al. 2011) at z = 0.106, WiggleZ (Drinkwater et al. 2010; Blake et al. 2011b; Kazin et al. 2014) at z = 0.44, 0.6, 0.73, and Baryon…”
BackgroundInfluentialTroxel, M. A., & Ishak, M. (2014) · Physics Reports · doi:10.1016/j.physrep.2014.11.001 · Cited by 289
“This model has been supported by a wide range of observations, including the cosmic microwave background (CMB) (Fowler et al., 2010; Das et al., 2011; Keisler et al., 2011; Reichardt et al., 2012; Ade et al., 2013a; Hinshaw et al., 2013), baryon acoustic oscillations (BAO) (Beutler et al., 2011; Anderson et al., 2012;…”
BackgroundInfluentialPlanck 2018 results. I. Overview and the cosmological legacy of Planck
Collaboration, P., Akrami, Y., Arroja, F. M. A., Ashdown, M., Aumont, J., Baccigalupi, C., Ballardini, M., Banday, A. J., Barreiro, R. B., Bartolo, N., et al. (2020) · Technical University of Denmark, DTU Orbit (Technical University of Denmark, DTU) · doi:10.17863/cam.33674 · Cited by 374
A lower bound on the mass of cold thermal dark matter from Planck
Bœhm, C., Dolan, M. J., & McCabe, C. (2013) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2013/08/041 · Cited by 279
Howlett, C., Ross, A. J., Samushia, L., Percival, W. J., & Manera, M. (2015) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stu2693 · Cited by 276
“This sampling positions the galaxies redshift between BOSS LOWZ, and the 6-degree Field Galaxy Survey (6dFGS; Beutler et al. 2011), filling in a gap in the chain of measurements at different redshifts.”
DESI 2024 III: baryon acoustic oscillations from galaxies and quasars
Adame, A. G., Aguilar, J., Ahlen, S. P., Alam, S., Alexander, D. M., Alvarez, M. A., Alves, O., Anand, A., Andrade, U., Armengaud, E., et al. (2025) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2025/04/012 · Cited by 275
Self-citationDark Energy Survey Year 1 Results: Cosmological constraints from cluster abundances and weak lensing
Abbott, T., Aguena, M., Alarcon, A., Allam, S., Allen, S., Annis, J., Ávila, S., Bacon, D., Bechtol, K., Bermeo, A., et al. (2020) · Physical Review D · doi:10.1103/physrevd.102.023509 · Cited by 115
Dark Energy Survey Year 1 Results: A Precise H0 Estimate from DES Y1, BAO, and D/H Data
Abbott, T. M. C., Abdalla, F. B., Annis, J. T., Bechtol, K., Blazek, J., Benson, B. A., Bernstein, R. A., Bernstein, G. M., Bertin, E., Brooks, D., et al. (2018) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/sty1939 · Cited by 273
“…as Type Ia supernovae (SNe) (e.g. Betoule et al. 2014); galaxy–galaxy (gg) clustering in the late-time Universe (e.g. Gaztañaga, Cabré & Hui 2009; Beutler et al. 2011; Ross et al. 2015; Alam et al. 2017); the time delays of multiply imaged quasars (e.g. Bonvin et al. 2017); and weak…”
BackgroundMethodInfluentialAbbott, T. M. C., Allam, S., Andersen, P., Angus, C., Asorey, J., Avelino, A., Avila, S., Bassett, B. A., Bechtol, K., Bernstein, G. M., et al. (2019) · The Astrophysical Journal Letters · doi:10.3847/2041-8213/ab04fa · Cited by 273
“Adding a BAO prior (Alam et al. 2017; Ross et al. 2015; Beutler et al. 2011) in addition to the CMB prior and SN constraints, our best fit w-value (Table 2, row 7) is shifted by only 0.006, the uncertainty is reduced by ∼ 20% compared to our primary result, and the evidence ratio between SN+CMB and…”
ResultInfluentialEvidence for Massive Neutrinos from Cosmic Microwave Background and Lensing Observations
Battye, R. A., & Moss, A. (2014) · Physical Review Letters · doi:10.1103/physrevlett.112.051303 · Cited by 271
Baryon acoustic oscillations at z = 2.34 from the correlations of Lyα absorption in eBOSS DR14
Agathe, V. D. S., Balland, C., Bourboux, H. D. M. D., Busca, N. G., Blomqvist, M., Guy, J., Rich, J., Font-Ribera, A., Pieri, M. M., Bautista, J., et al. (2019) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201935638 · Cited by 270
“…victoria.de.sainte.agathe@lpnhe.in2p3.fr Most BAO measurements have employed discrete objects like galaxies (Percival et al. 2010; Reid et al. 2010; Beutler et al. 2011; Blake et al. 2011; Anderson et al. 2012, 2014a,b; Ross et al. 2015; Alam et al. 2017; Bautista et al. 2018) or quasars (Ata et…”
BackgroundInfluentialSamushia, L., Reid, B., White, M. J., Percival, W. J., Cuesta, A. J., Zhao, G., Ross, A. J., Manera, M., Aubourg, É., Beutler, F., et al. (2014) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stu197 · Cited by 264
“Recent highlights include the BAO measurements from the 6dF Galaxy Redshift Survey (6dFGRS; Beutler et al. 2011), Sloan Digital Sky Survey II (SDSS-II; Padmanabhan et al. 2012), SDSS-III Baryon Oscillation Spectroscopic Survey (BOSS) Data Release 9 sample (DR9; Anderson et al. 2012), WiggleZ survey…”
MethodSelf-citationBourboux, H. M. D. M. D., Goff, J. L., Blomqvist, M., Busca, N., Guy, J., Rich, J., Yéche, C., Bautista, J., Burtin, É., Dawson, K., et al. (2017) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201731731 · Cited by 245
“02 22 5v 3 [ as Beutler et al. 2011; Blake et al. 2011; Padmanabhan et al. 2012; Mehta et al. 2012; Chuang & Wang 2012; Xu et al. 2013; Ross et al. 2015) map distances and expansion rates for z < 0.8.”
BackgroundInfluentialBaryon acoustic oscillations from the cross-correlation of Ly α absorption and quasars in eBOSS DR14
Blomqvist, M., Bourboux, H. D. M. D., Busca, N. G., Agathe, V. D. S., Rich, J., Balland, C., Bautista, J., Dawson, K., Font-Ribera, A., Guy, J., et al. (2019) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201935641 · Cited by 268
“(50) and (51)), the galaxy data of Alam et al. (2017), Beutler et al. (2011) Ross et al. (2015) and Bautista et al. (2018) and the quasar data of Ata et al. (2018) yields ΩM = 0.293 ± 0.027, ΩΛ = 0.675 ± 0.099 (53) corresponding to Ωk = 0.032 ± 0.117.”
MethodInfluentialBeutler, F., Seo, H., Ross, A. J., McDonald, P., Saito, S., Bolton, A. S., Brownstein, J. R., Chuang, C.-H., Cuesta, A. J., Eisenstein, D. J., et al. (2016) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stw2373 · Cited by 267
“The WiggleZ survey extended these early detections to higher redshifts (Blake et al. 2011; Kazin et al. 2014), while the 6dF Galaxy Survey (6dFGS) measured the BAO signal at z = 0.1 (Beutler et al. 2011).”
BackgroundInfluentialSelf-citationAddison, G. E., Watts, D. J., Bennett, C. L., Halpern, M., Hinshaw, G., & Weiland, J. L. (2018) · The Astrophysical Journal · doi:10.3847/1538-4357/aaa1ed · Cited by 265
Cosmic microwave background bounds on primordial black holes including dark matter halo accretion
Serpico, P. D., Poulin, V., Inman, D., & Kohri, K. (2020) · Physical Review Research · doi:10.1103/physrevresearch.2.023204 · Cited by 265
Lombriser, L., & Lima, N. A. (2017) · Physics Letters B · doi:10.1016/j.physletb.2016.12.048 · Cited by 261
Union through UNITY: Cosmology with 2000 SNe Using a Unified Bayesian Framework
Rubin, D., Aldering, G., Betoule, M., Fruchter, A., Huang, X., Kim, A., Lidman, C. E., Linder, E. V., Perlmutter, S., Ruiz-Lapuente, P., et al. (2025) · The Astrophysical Journal · doi:10.3847/1538-4357/adc0a5 · Cited by 505
Acoustic dark energy: Potential conversion of the Hubble tension
Lin, M., Benevento, G., Hu, W., & Raveri, M. (2019) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.100.063542 · Cited by 257
Efstathiou, G. (2021) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stab1588 · Cited by 251
From cosmic deceleration to acceleration: new constraints from SN Ia and BAO/CMB
Giostri, R., dos Santos, M. V., Waga, I., Reis, R. R. R., Calvão, M. O., & Lago, B. L. (2012) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2012/03/027 · Cited by 261
“In [19] the 6dF Galaxy Survey also reported a new measurement of rs/DV at z = 0.106 and, more recently, the WiggleZ team [7] obtained results at z = 0.44, z = 0.60 and z = 0.73 (see table 1).”
InfluentialDriver, S. P., Bellstedt, S., Robotham, A. S. G., Baldry, I. K., Davies, L. J. M., Liske, J., Obreschkow, D., Taylor, E. N., Wright, A. H., Alpaslan, M., et al. (2022) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stac472 · Cited by 252
Self-citationTroxel, M. A., & Ishak, M. (2016) · Cited by 243
Cosmology and astrophysics from relaxed galaxy clusters – II. Cosmological constraints
Mantz, A. B., Allen, S. W., Morris, R. G., Rapetti, D., Applegate, D., Kelly, P. L., von der Linden, A., & Schmidt, R. W. (2014) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stu368 · Cited by 248
“In addition, we include the Union 2.1 compilation of type Ia supernovae (Suzuki et al. 2012) and BAO data from the combination of results from the 6-degree Field Galaxy Survey (6dFGS; z = 0.106; Beutler et al. 2011) and the Sloan Digital Sky Survey (z = 0.35 and 0.57; Padmanabhan et al. 2012; Anderson et al. 2014).”
BackgroundInfluentialWALLABY – an SKA Pathfinder H i survey
Koribalski, B. S., Staveley‐Smith, L., Westmeier, T., Serra, P., Spekkens, K., Wong, O. I., Lee-Waddell, K., Lagos, C. D. P., Obreschkow, D., Ryan-Weber, E. V., et al. (2020) · Astrophysics and Space Science · doi:10.1007/s10509-020-03831-4 · Cited by 244
“We expect to accurately measure the density-dependence of the H I mass function, the clustering and bias parameter for gas-rich galaxies and the local flow field (e.g., Beutler et al. 2011; Papastergis et al. 2013).”
MethodSelf-citationAylor, K., Joy, M., Knox, L., Millea, M., Raghunathan, S., & Wu, W. L. K. (2019) · The Astrophysical Journal · doi:10.3847/1538-4357/ab0898 · Cited by 243
“We do not include any other BAO data, such as that from the 6df galaxy survey (Beutler et al. 2011) or a BOSS DR12 Lyα absorption cross-correlation analysis (du Mas des Bourboux et al. 2017).”
BackgroundMethodRobust weak-lensing mass calibration of Planck galaxy clusters
von der Linden, A., Mantz, A., Allen, S. W., Applegate, D. E., Kelly, P. L., Morris, R. G., Wright, A., Allen, M. T., Burchat, P. R., Burke, D. L., et al. (2014) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stu1423 · Cited by 241
Why reducing the cosmic sound horizon alone can not fully resolve the Hubble tension
Jedamzik, K., Pogosian, L., & Zhao, G.-B. (2021) · Communications Physics · doi:10.1038/s42005-021-00628-x · Cited by 237
Gariazzo, S., Giunti, C., Laveder, M., Li, Y. F., & Zavanin, E. M. (2015) · Journal of Physics G Nuclear and Particle Physics · doi:10.1088/0954-3899/43/3/033001 · Cited by 236
Vagnozzi, S., Dhawan, S., Gerbino, M., Freese, K., Goobar, A., & Mena, O. (2018) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.98.083501 · Cited by 255
H i intensity mapping: a single dish approach
Battye, R. A., Browne, I. W. A., Dickinson, C., Heron, G. A., Maffei, B., & Pourtsidou, A. (2013) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stt1082 · Cited by 235
“…of the SDSS Luminous Red Galaxy (LRG) survey (Eisenstein et al. 2005), subsequent detections have been reported by a number of groups analysing data from 2dF (Cole et al. 2005), SDSS DR7 (Percival et al. 2010), WiggleZ (Blake et al. 2011), 6dF (Beutler et al. 2011) and BOSS (Anderson et al. 2012).”
MethodConcordance and discordance in cosmology
Raveri, M., & Hu, W. (2019) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.99.043506 · Cited by 230
Macaulay, E., Nichol, R. C., Bacon, D., Brout, D., Davis, T. M., Zhang, B. R., Bassett, B. A., Scolnic, D. M., Möller, A., D’Andrea, C. B., et al. (2019) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stz978 · Cited by 230
Poulin, V., Smith, T. L., & Karwal, T. (2023) · Physics of the Dark Universe · doi:10.1016/j.dark.2023.101348 · Cited by 234
“[161] Florian Beutler, Chris Blake, Matthew Colless, D.”
BackgroundEcho of interactions in the dark sector
Kumar, S., & Nunes, R. C. (2017) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.96.103511 · Cited by 229
Is the Hubble tension a hint of AdS phase around recombination?
Ye, G., & Yun-song Piao, A. (2020) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.101.083507 · Cited by 224
Anderson, L., Aubourg, É., Bailey, S., Beutler, F., Bolton, A. S., Brinkmann, J., Brownstein, J. R., Chuang, C.-H., Cuesta, A. J., Dawson, K., et al. (2014) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stt2206 · Cited by 224
“…information from anisotropic clustering from surveys covering different redshift ranges: such as the low-redshift BAO measurements of the 6dF Galaxy Survey (Beutler et al. 2011) to the high-redshift Lyman α forest clustering results (Busca et al. 2012; Slosar et al. 2013; Kirkby et al. 2013).”
BackgroundInfluentialSelf-citationResolving the Hubble tension with new early dark energy
Niedermann, F., & Sloth, M. S. (2020) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.102.063527 · Cited by 254
“The 6dF Galaxy Survey: baryon acoustic oscillations and the local Hubble constant.”
MethodInfluentialOka, A., Saito, S., Nishimichi, T., Taruya, A., & Yamamoto, K. (2014) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stu111 · Cited by 223
“…gigantic galaxy redshift surveys are designed to detect the baryon acoustic oscillation (BAO) scale that is used as a standard ruler to explore the expansion history (Anderson et al. 2012; Beutler et al. 2011; Blake et al. 2011c; Eisenstein et al. 2005b; Percival et al. 2007a; Seo et al. 2012).”
MethodZhao, G., Wang, Y., Saito, S., Gil-Marín, H., Percival, W. J., Wang, D., Chuang, C.-H., Ruggeri, R., Mueller, E.-M., Zhu, F., et al. (2018) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/sty2845 · Cited by 223
“…Lyman-α auto- and cross-correlation BAO measurements (Gontcho et al. 2018) and the isotropic BAO measurements using MGS (Ross et al. 2015) and 6dFGS (Beutler et al. 2011) samples, significantly improves the constraint, namely, a Universe without dark energy is excluded at 7.37σ by these BAO…”
BackgroundMethodSelf-citationDistance priors from Planck final release
Chen, L., Huang, Q.-G., & Wang, K. (2019) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2019/02/028 · Cited by 223
“We use the 6dFGS [33], SDSS-MGS [34] and the final DR12 anisotropic BAO data [35] at z = 0.”
MethodA Simple Phenomenological Emergent Dark Energy Model can Resolve the Hubble Tension
Li, X., & Shafieloo, A. (2019) · The Astrophysical Journal Letters · doi:10.3847/2041-8213/ab3e09 · Cited by 223
“(ii) BAOs: four lower redshift BAO data sets are used: 6-degree Field Galaxy Survey (6dFGS) (Beutler et al. 2011), the SDSS Data Release 7 Main Galaxy sample (MGS) (Ross et al. 2015), the BOSS DR12 galaxies (Alam et al. 2017a) and the eBOSS DR14 quasars (Zhao et al. 2018).”
MethodUnfinished fabric of the three neutrino paradigm
Capozzi, F., Valentino, E. D., Lisi, E., Marrone, A., MELCHIORRI, A., & Palazzo, A. (2021) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.104.083031 · Cited by 223
Towards a cosmological neutrino mass detection
Allison, R., Caucal, P., Calabrese, E., Dunkley, J., & Louis, T. (2015) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.92.123535 · Cited by 220
First Evidence of Running Cosmic Vacuum: Challenging the Concordance Model
Solà, J., Gómez-Valent, A., & Pérez, J. D. C. (2017) · The Astrophysical Journal · doi:10.3847/1538-4357/836/1/43 · Cited by 220
“S2) 5 points on the isotropic BAO estimator rs(zd)/DV (zi): z = 0.106 (Beutler et al. 2011), z = 0.15 (Ross et al. 2015), zi = 0.44, 0.6, 0.73 (Kazin et al. 2014), with the correlations between the last 3 points.”
BackgroundInfluentialGeorge, E. M., Reichardt, C. L., Aird, K. A., Benson, B. A., Bleem, L. E., Carlstrom, J. E., Chang, C. L., Cho, H.-M., Crawford, T. M., Crites, A. T., et al. (2015) · The Astrophysical Journal · doi:10.1088/0004-637x/799/2/177 · Cited by 219
“We include measurements of the BAO feature from SDSS (Anderson et al. 2012; Padmanabhan et al. 2012) and 6dF data (Beutler et al. 2011).”
MethodRock ‘n’ roll solutions to the Hubble tension
Agrawal, P., Cyr-Racine, F.-Y., Pinner, D., & Randall, L. (2023) · Physics of the Dark Universe · doi:10.1016/j.dark.2023.101347 · Cited by 217
“We also include low-z BAO measurements from the 6dF Galaxy Survey [149] and from the Main Galaxy Sample (MGS) of SDSS [150].”
MethodSamushia, L., Reid, B., White, M. J., Percival, W. J., Cuesta, A. J., Lombriser, L., Manera, M., Nichol, R. C., Schneider, D. P., Bizyaev, D., et al. (2012) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/sts443 · Cited by 218
Cosmological parameters derived from the final Planck data release (PR4)
Tristram, M., Banday, A. J., Douspis, M., Garrido, X., Gorski, K. M., Versillé, S., Hergt, L. T., Ilić, S., Keskitalo, R., Lagache, G., et al. (2023) · Astronomy and Astrophysics · doi:10.1051/0004-6361/202348015 · Cited by 217
“This includes data from 6dF (Beutler et al. 2011), SDSS DR7 (specifically MGS, Ross et al. 2015), and SDSS DR16 (LRG, ELG, QSO, Ly-α auto, and Ly-α xQSO, Alam et al. 2021), which also incorporates some constraints on the growth of structures through redshift-space distortions.”
BackgroundMethodLyman-alpha forests cool warm dark matter
Baur, J., Palanque‐Delabrouille, N., Yèche, C., Magneville, C., & Viel, M. (2016) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2016/08/012 · Cited by 216
“We thus also include, in a second step, the Planck temperature data at low and high multipoles (PlanckTT), the low-multipole HFI-based polarization data up to ` = 29 (‘lowP’), and the ` ≥ 30 polarization data (denoted ‘TE’ and ‘EE’), as well as measurements of the BAO scale by 6dFGS [53], the main galaxy sample of SDS…”
MethodProbing the interaction between dark matter and dark energy in the presence of massive neutrinos
Kumar, S., & Nunes, R. C. (2016) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.94.123511 · Cited by 216
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
“Figure 7 shows constraints in the Ωm −H0 plane for the BAO constraint from combining BOSS CMASS with the BOSS ‘LOWZ’ sample (Anderson et al. 2014), Sloan Digital Sky Survey Main Galaxy Sample (Ross et al. 2015, SDSS MGS), and Six-degreeField Galaxy Survey (Beutler et al. 2011, 6dFGS) measurements.”
MethodMeasuring DA and H at z=0.35 from the SDSS DR7 LRGs using baryon acoustic oscillations
Xu, X., Cuesta, A. J., Padmanabhan, N., Eisenstein, D. J., & McBride, C. K. (2013) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stt379 · Cited by 214
“…(Cole et al. 2005; Eisenstein et al. 2005; Hütsi 2006; Tegmark et al. 2006; Percival et al. 2007; Kazin et al. 2010a; Percival et al. 2010; Beutler et al. 2011; Blake et al. 2011a; Mehta et al. 2012; Padmanabhan et al. 2012; Xu et al. 2012), which only allow us to measure the spherically…”
BackgroundRefined bounds on MeV-scale thermal dark sectors from BBN and the CMB
Sabti, N., Alvey, J., Escudero, M., Fairbairn, M., & Blas, D. (2020) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2020/01/004 · Cited by 234
The WiggleZ Dark Energy Survey: the transition to large-scale cosmic homogeneity
Scrimgeour, M. I., Davis, T. M., Blake, C., James, J. B., Poole, G. B., Staveley‐Smith, L., Brough, S., Colless, M., Contreras, C., Couch, W., et al. (2012) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2012.21402.x · Cited by 239
“A homogeneity scale below 100 h−1Mpc may also seem to contradict the fact that the correlation function has a known feature, the Baryon Acoustic Oscillation (BAO) peak at ∼ 105 h−1Mpc (Eisenstein et al. 2005; Percival et al. 2010; Beutler et al. 2011; Blake et al. 2011c).”
BackgroundSelf-citationPan, S., Yang, W., Valentino, E. D., Saridakis, E. N., & Chakraborty, S. (2019) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.100.103520 · Cited by 205
“• We use the Baryon acoustic oscillations (BAO) distance measurements from the following references [109, 110, 111].”
MethodNiedermann, F., & Sloth, M. S. (2021) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.103.l041303 · Cited by 257
Planck 2018 resultsPreprint
Aghanim, N., Akrami, Y., Ashdown, M., Aumont, J., Baccigalupi, C., Ballardini, M., Banday, A. J., Barreiro, R. B., Bartolo, N., Basak, S., et al. (2018) · arXiv (Cornell University) · doi:10.17863/cam.104203 · Cited by 210
Signatures of f ( Q ) gravity in cosmology
Frusciante, N. (2021) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.103.044021 · Cited by 207
Current unknowns in the three-neutrino framework
Capozzi, F., Lisi, E., Marrone, A., & Palazzo, A. (2018) · Progress in Particle and Nuclear Physics · doi:10.1016/j.ppnp.2018.05.005 · Cited by 242
Constraining the Self-Interacting Neutrino Interpretation of the Hubble Tension
Blinov, N., Kelly, K. J., Krnjaic, G., & McDermott, S. D. (2019) · Physical Review Letters · doi:10.1103/physrevlett.123.191102 · Cited by 205
Baryon Acoustic Oscillations and the Hubble constant: past, present and future
Cuceu, A., Farr, J., Lemos, P., & Font-Ribera, A. (2019) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2019/10/044 · Cited by 205
Relieving the Hubble Tension with Primordial Magnetic Fields
Jedamzik, K., & Pogosian, L. (2020) · Physical Review Letters · doi:10.1103/physrevlett.125.181302 · Cited by 205
corrfunc – a suite of blazing fast correlation functions on the CPU
Sinha, M., & Garrison, L. H. (2019) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stz3157 · Cited by 204
“For example, the 2PCF has been used to constrain the cosmological model (Eisenstein et al. 2005; Tegmark et al. 2006; Blake et al. 2011; Beutler et al. 2011; Percival et al. 2010; Anderson et al. 2014; Hildebrandt et al. 2017; Alam et al. 2017), dissecting halo clustering (e.g., Gao et al. 2005;…”
MethodThe Atacama Cosmology Telescope: DR6 constraints on extended cosmological models
Calabrese, E., Hill, J. C., Jense, H. T., Posta, A. L., Abril-Cabezas, I., Addison, G. E., Ade, P. A. R., Aiola, S., Alford, T., Alonso, D., et al. (2025) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2025/11/063 · Cited by 204
Constraints on neutrino masses from Lyman-alpha forest power spectrum with BOSS and XQ-100
Yèche, C., Palanque‐Delabrouille, N., Baur, J., & Bourboux, H. D. M. D. (2017) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2017/06/047 · Cited by 203
“We occasionally combine CMB data with measurements of the BAO scale by 6dFGS [30], SDSS main galaxy sample [31], BOSS-LOWZ [32] and CMASS-DR11 [32].”
MethodThe BAO+BBN take on the Hubble tension
Schöneberg, N., Julien Lesgourgues, A., & Hooper, D. C. (2019) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2019/10/029 · Cited by 203
“ll extend our analysis to the case of a free N e in subsection3.2. Our conclusions are presented in section4. { 3 { Measurement z BAO Value Ref. BAO from galactic data 6DF 0.106 r s=D V = 0:327 0:015 [38] SDSS DR7 MGS 0.15 D V=r s= 4:47 0:16 [39] SDSS DR14 eBOSS QSO 1.52 D V=r s= 26:0 1:0 [40] SDSS DR12 galaxies 0.38,…”
BackgroundInfluentialThe evidence for a spatially flat Universe
Efstathiou, G., & Gratton, S. (2020) · Monthly Notices of the Royal Astronomical Society: Letters · doi:10.1093/mnrasl/slaa093 · Cited by 203
“…in Planck Collaboration et al. (2018b); ‘Pantheon’ denotes use of the Pantheon Type Ia supernovae sample of (Scolnic et al. 2015); ‘BAO’ denotes use of the baryonic acoustic oscillation measurements from Beutler et al. (2011); Ross et al. (2015); Alam et al. (2017) as discussed in PCP18 and EG.”
MethodImplications of an extended dark energy cosmology with massive neutrinos for cosmological tensions
Poulin, V., Boddy, K. K., Bird, S., & Kamionkowski, M. (2018) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.97.123504 · Cited by 201
“[40] Florian Beutler, Chris Blake, Matthew Colless, D.”
BackgroundThe VIMOS Public Extragalactic Redshift Survey (VIPERS)
Pezzotta, A., de la Torre, S., Bel, J., Granett, B. R., Guzzo, L., Peacock, J. A., Garilli, B., Scodeggio, M., Bolzonella, M., Abbas, U., et al. (2017) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201630295 · Cited by 198
“…microwave background anisotropies (Hinshaw et al. 2012; Planck Collaboration et al. 2015), baryon acoustic oscillations in the galaxy distribution (Beutler et al. 2011; Blake et al. 2011; Anderson et al. 2012), to SNe Ia luminosity distances (Riess et al. 1998; Perlmutter et al. 1999), require…”
BackgroundSánchez, A. G., Scóccola, C. G., Ross, A. J., Percival, W. J., Manera, M., Montesano, F., Mazzalay, X., Cuesta, A. J., Eisenstein, D. J., Kazin, E. A., et al. (2012) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2012.21502.x · Cited by 198
“…al. (2005) and has been subsequently observed using a variety of datasets and techniques (Hütsi 2006; Padmanabhan et al. 2007; Percival et al. 2007, 2010; Cabré & Gaztañaga 2009; Gaztañaga et al. 2009; Kazin et al. 2010; Beutler et al. 2011; Blake et al. 2011; Ho et al. 2012; Seo et al. 2012).”
BackgroundMethodInfluentialNumerical simulations of the dark universe: State of the art and the next decade
Kuhlen, M., Vogelsberger, M., & Angulo, R. E. (2012) · Physics of the Dark Universe · doi:10.1016/j.dark.2012.10.002 · Cited by 222
Camarena, D., & Marra, V. (2021) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stab1200 · Cited by 194
Chuang, C.-H., Kitaura, F.-S., Prada, F., Zhao, C., & Yepes, G. (2014) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stu2301 · Cited by 195
“Alternatively, log-normal mock catalogues (Coles & Jones 1991) have been widely used (e.g., Cole et al. 2005; Percival et al. 2010; Reid et al. 2010; Blake et al. 2011; Beutler et al. 2011).”
MethodHubble sinks in the low-redshift swampland
Banerjee, A., Cai, H., Heisenberg, L., Colgáin, E. Ó., Sheikh-Jabbari, M. M., & Yang, T. (2021) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.103.l081305 · Cited by 195
Wang, Y., Zhao, G., Chuang, C.-H., Ross, A. J., Percival, W. J., Gil-Marín, H., Cuesta, A. J., Kitaura, F.-S., Rodríguez-Torres, S. A., Brownstein, J. R., et al. (2017) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stx1090 · Cited by 195
Galileon gravity in light of ISW, CMB, BAO and H 0 data
Renk, J. J., Zumalacárregui, M., Montanari, F., & Barreira, A. (2017) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2017/10/020 · Cited by 192
“BAO scale measurements at lower redshift8 that includes SDSS DR7 LRG [34], BOSS DR9 CMASS [35] and the 6dF Galaxy Survey [36].”
BackgroundMethodInfluentialConstraining dark energy dynamics in extended parameter space
Valentino, E. D., MELCHIORRI, A., Linder, E. V., & Silk, J. I. (2017) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.96.023523 · Cited by 192
Revisiting a Negative Cosmological Constant from Low-Redshift Data
Visinelli, L., Vagnozzi, S., & Danielsson, U. (2019) · Symmetry · doi:10.3390/sym11081035 · Cited by 183
D’Eramo, F., Ferreira, R. Z., Notari, A., & Bernal, J. L. (2018) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2018/11/014 · Cited by 189
Mock galaxy catalogues using the quick particle mesh method
White, M. J., Tinker, J. L., & McBride, C. K. (2013) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stt2071 · Cited by 193
“This model has been used to generate mock catalogues for analyses of the 2dF (e.g. Cole et al. 2005), SDSS (most recently, Percival et al. 2010; Reid et al. 2010), WiggleZ (Blake et al. 2011) and 6dF (Beutler et al. 2011, 2012) surveys, among others.”
MethodAbbott, T. M. C., Abdalla, F. B., Alarcon, A., Allam, S., Andrade-Oliveira, F., Annis, J. T., Avila, S., Banerji, M., Banik, N., Bechtol, K., et al. (2018) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/sty3351 · Cited by 188
“…& et al. 2010; Ross et al. 2015a; Alam et al. 2016; Ata & et al. 2017; Delubac et al. 2015; Bautista et al. 2017a), the 2-degree Field Galaxy Redshift Survey (Percival et al. 2001; Cole et al. 2005), WiggleZ (Blake et al. 2011), and the 6-degree Field Galaxy Survey (6dFGS, Beutler et al. 2011).”
BackgroundNeutrino Mass Ordering from Oscillations and Beyond: 2018 Status and Future Prospects
de Salas, P. F., Gariazzo, S., Mena, O., Ternes, C. A., & Tórtola, M. (2018) · Frontiers in Astronomy and Space Sciences · doi:10.3389/fspas.2018.00036 · Cited by 188
Interacting dark energy with time varying equation of state and the H0 tension
Yang, W., Mukherjee, A., Valentino, E. D., & Pan, S. (2018) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.98.123527 · Cited by 188
“• Baryon acoustic oscillations (BAO) distance measurements [58, 59, 60].”
BackgroundVagnozzi, S. (2021) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.104.063524 · Cited by 192
Can late dark energy transitions raise the Hubble constant?
Benevento, G., Hu, W., & Raveri, M. (2020) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.101.103517 · Cited by 187
Accelerated expansion from ghost-free bigravity: a statistical analysis with improved generality
Akrami, Y., Koivisto, T., & Sandstad, M. (2013) · Journal of High Energy Physics · doi:10.1007/jhep03(2013)099 · Cited by 191
Current unknowns in the three neutrino framework
Capozzi, F., Lisi, E., Marrone, A., & Palazzo, A. (2018) · MPG.PuRe (Max Planck Society) · Cited by 184
Constraints on large-scale dark acoustic oscillations from cosmology
Cyr-Racine, F.-Y., de Putter, R., Raccanelli, A., & Sigurdson, K. (2014) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.89.063517 · Cited by 183
Arbitrating the S 8 discrepancy with growth rate measurements from redshift-space distortions
Nunes, R. C., & Vagnozzi, S. (2021) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stab1613 · Cited by 179
Improvement of cosmological neutrino mass bounds
Giusarma, E., Gerbino, M., Mena, O., Vagnozzi, S., Ho, S., & Katherine Freese, B. (2016) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.94.083522 · Cited by 181
A non-linear solution to the S 8 tension?
Amon, A., & Efstathiou, G. (2022) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stac2429 · Cited by 181
Akarsu, Ö., Kumar, S., Myrzakulov, R., Sami, M., & Xu, L. (2014) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2014/01/022 · Cited by 180
Does Hubble tension signal a breakdown in FLRW cosmology?
Krishnan, C., Mohayaee, R., Colgáin, E. Ó., Sheikh-Jabbari, M. M., & Yin, L. (2021) · Classical and Quantum Gravity · doi:10.1088/1361-6382/ac1a81 · Cited by 179
Structure formation in f(T) gravity and a solution for H0 tension
Nunes, R. C. (2018) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2018/05/052 · Cited by 177
“BAO: The baryon acoustic oscillations (BAO) measurements from the Six Degree Field Galaxy Survey (6dF) [74], the Main Galaxy Sample of Data Release 7 of Sloan Digital Sky Survey (SDSS-MGS) [75], the LOWZ and CMASS galaxy samples of the Baryon Oscillation Spectroscopic Survey (BOSS-LOWZ and BOSS-CMASS, respectively) [7…”
MethodInteracting dark sector and precision cosmology
Buen-Abad, M. A., Schmaltz, M., Julien Lesgourgues, A., & Brinckmann, T. (2018) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2018/01/008 · Cited by 176
Can the H 0 tension be resolved in extensions to ΛCDM cosmology?
Guo, R.-Y., Zhang, J.-F., & Zhang, X. (2019) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2019/02/054 · Cited by 176
“106 [80], and the Main Galaxy Sample of Data Release 7 of Sloan Digital Sky Survey at zeff = 0.”
BackgroundH0 tension, phantom dark energy, and cosmological parameter degeneracies
Alestas, G., Kazantzidis, L., & Perivolaropoulos, L. (2020) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.101.123516 · Cited by 174
“[72] Florian Beutler, Chris Blake, Matthew Colless, D.”
BackgroundMethod
Metadata
- 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
- 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)
- 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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