The DOI matches its Crossref record; 87 of the 87 references it cites were found in a registry or an index.
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.
Overview
The claims and statistics of this paper haven’t been checked yet.
Run the check — free, no account needed. It reads the open-access text and checks the sources it cites.
Integrity signals
Registry
Cites
Statistics
Verification
Claims the paper makes
The claims and statistics of this paper haven’t been checked yet.
Run the check — free, no account needed. It reads the open-access text and checks the sources it cites.
Self-check
Percentages, sums and reported differences re-computed from the paper’s own numbers.
The self-check needs the paper’s full text.
Citations
Cites
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
Cited by
Sorted by citations
Planck 2018 results: VI. Cosmological parameters
Planck Collaboration, Aghanim, N., Akrami, Y., Ashdown, M., Aumont, J., Baccigalupi, C., Ballardini, M., Banday, A. J., Barreiro, R. B., Bartolo, N., et al. (2020) · Astronomy & Astrophysics · doi:10.1051/0004-6361/201833910 · Cited by 14,258
Ade, P. A. R., Aghanim, N., Arnaud, M., Ashdown, M., Aumont, J., Baccigalupi, C., Banday, A. J., Barreiro, R. B., Bartlett, J. G., Bartolo, N., et al. (2016) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201525830 · Cited by 10,685
“XIII. shows DV/rdrag from the analysis of Anderson et al. (2014), updating the BOSS-DR9 analysis of Anderson et al. (2012) used in PCP13.”
InfluentialPlanck 2013 results. XVI. Cosmological parameters
Ade, P. A. R., Aghanim, N., Armitage-Caplan, C., Arnaud, M., Ashdown, M., Atrio-Barandela, F., Aumont, J., Baccigalupi, C., Banday, A. J., Barreiro, R. B., et al. (2014) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201321591 · Cited by 8,459
Ade, P. A. R., Aghanim, N., Arnaud, M., Ashdown, M., Aumont, J., Baccigalupi, C., Banday, A. J., Barreiro, R. B., Bartlett, J. G., Bartolo, N., et al. (2016) · Research at the University of Copenhagen (University of Copenhagen) · doi:10.17863/cam.32861 · Cited by 5,299
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
“At lower redshift, z = 0.1, a detection of the BAO scale has been made using the 6dFGS survey (Beutler et al. 2011).”
BackgroundMethodInfluentialPlanck 2018 results. VI. Cosmological parametersPreprint
Planck Collaboration, Aghanim, N., Akrami, Y., Ashdown, M., Aumont, J., Baccigalupi, C., Ballardini, M., Banday, A. J., Barreiro, R. B., Bartolo, N., et al. (2018) · arXiv (Cornell University) · doi:10.48550/arxiv.1807.06209 · Cited by 3,364
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
“Symbols show BAO measurements from z ≈ 0.1 to z ≈ 2.2 collected from 6dFGS (Beutler et al. 2011), SDSS-I/II (Percival et al. 2010; Ross et al. 2015), WiggleZ (Blake et al. 2011a,b), and the BOSS Lyα forest autoand cross-correlations (Delubac et al. 2015 and Font-Ribera et al. 2014, respectively),…”
MethodInfluentialSelf-citationNine-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Parameter Results
WRIGHT, E. L. (2016) · NASA STI Repository (National Aeronautics and Space Administration) · doi:10.15781/t2st7f05x · Cited by 2,604
Akrami, Y., Arroja, F. M. A., Ashdown, M., Aumont, J., Baccigalupi, C., Ballardini, M., Banday, A. J., Barreiro, R. B., Bartolo, N., Basak, S., et al. (2019) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201833887 · Cited by 2,435
“For our BAO data compilation, we use the measurements of DV/rd from the 6dF survey at an effective redshift zeff = 0.106 (Beutler et al. 2011), and the SDSS Main Galaxy Sample at zeff = 0.15 (Ross et al. 2015), plus the final interpreta- tion of the SDSS III DR12 data (Alam et al. 2016), with…”
BackgroundMethodInfluentialTHE BARYON OSCILLATION SPECTROSCOPIC SURVEY OF SDSS-III
Dawson, K. S., Schlegel, D. J., Ahn, C. P., Anderson, S. F., Aubourg, É., Bailey, S., Barkhouser, R. H., Bautista, J., Beifiori, A., Berlind, A. A., et al. (2012) · The Astronomical Journal · doi:10.1088/0004-6256/145/1/10 · Cited by 2,018
“75 National Astronomy Observatories, Chinese Academy of Science, Beijing, 100012, P. R. China. a 4.5% BAO distance measurement at redshift z ∼ 0.1 (Beutler et al. 2011).”
BackgroundMethodInfluentialSelf-citationIn the realm of the Hubble tension—a review of solutions *
Di Valentino, E., Mena, O., Pan, S., Visinelli, L., Yang, W., Melchiorri, A., Mota, D. F., Riess, A. G., & Silk, J. (2021) · Classical and Quantum Gravity · doi:10.1088/1361-6382/ac086d · Cited by 2,065
Ade, P. A. R., Aghanim, N., Arnaud, M., Arroja, F. M. A., Ashdown, M., Aumont, J., Baccigalupi, C., Ballardini, M., Banday, A. J., Barreiro, R. B., et al. (2016) · ORCA Online Research @Cardiff (Cardiff University) · doi:10.17863/cam.52 · Cited by 2,497
Improved cosmological constraints from a joint analysis of the SDSS-II and SNLS supernova samples
Betoule, M., Kessler, R., Guy, J., Mosher, J., Hardin, D., Biswas, R., Astier, P., El-Hage, P., König, M., Kuhlmann, S. E., et al. (2014) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201423413 · Cited by 1,910
“The BAO scale has now been detected in the correlation function of various galaxy surveys (Eisenstein et al. 2005; Beutler et al. 2011; Blake et al. 2011; Anderson et al. 2012), as well as in the Lyα forest of distant quasars (Busca et al. 2013; Slosar et al. 2013).”
MethodInfluentialAnderson, L., Aubourg, É., Bailey, S., Beutler, F., Bhardwaj, V., Blanton, M. R., Bolton, A. S., Brinkmann, J., Brownstein, J. R., Burden, A., et al. (2014) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stu523 · Cited by 1,908
“Our BAO distance constraints are parametrized as described above as a measurement on DV/rs at z = 0.57; we augment these with the z = 0.35 measurement from Padmanabhan et al. (2012a) as well as the 6dF measurement at z = 0.106 (Beutler et al. 2011).”
BackgroundMethodInfluentialSelf-citationThe clustering of the SDSS DR7 main Galaxy sample – I. A 4 per cent distance measure at z=0.15
Ross, A. J., Samushia, L., Howlett, C., Percival, W. J., Burden, A., & Manera, M. (2015) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stv154 · Cited by 1,745
“These include three spherically-averaged measurements; our own MGS measurement at z = 0.15, Beutler et al. (2011) at z = 0.11, Tojeiro et al. (2014) at z = 0.32, and the anisotropic measurement of Anderson et al. (2014) at z = 0.57.”
BackgroundMethodInfluentialAghanim, N., Akrami, Y., Arroja, F. M. A., Ashdown, M., Aumont, J., Baccigalupi, C., Ballardini, M., Banday, A. J., Barreiro, R. B., Bartolo, N., et al. (2019) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201833880 · Cited by 2,386
f ( T ) teleparallel gravity and cosmology
Cai, Y.-F., Capozzıello, S., Laurentis, M. D., & Saridakis, E. N. (2016) · Reports on Progress in Physics · doi:10.1088/0034-4885/79/10/106901 · Cited by 1,685
Observational probes of cosmic acceleration
Weinberg, D. H., Mortonson, M. J., Eisenstein, D. J., Hirata, C. M., Riess, A. G., & Rozo, E. (2013) · Physics Reports · doi:10.1016/j.physrep.2013.05.001 · Cited by 1,520
“Beutler et al. (2011) report a 2.4σ detection from the 6-degree Field Galaxy Survey (6dFGS), which covered 17,000 deg2 of sky, obtaining a 4.5% distance measurement to z = 0.1.”
MethodInfluentialPlanck 2015. XX. Constraints on inflation
Ade, P. A. R., Aghanim, N., Arnaud, M., Arroja, F. M. A., Ashdown, M., Aumont, J., Baccigalupi, C., Ballardini, M., Banday, A. J., Barreiro, R. B., et al. (2015) · CERN Document Server (European Organization for Nuclear Research) · doi:10.1051/0004-6361/201525898 · Cited by 12
Alam, S., Aubert, M., Avila, S., Balland, C., Bautista, J. E., Bershady, M. A., Bizyaev, D., Blanton, M. R., Bolton, A. S., Bovy, J., et al. (2021) · Physical Review D · doi:10.1103/physrevd.103.083533 · Cited by 1,337
“…km s−1 Mpc−1 (Riess et al. 2011), and the BOSS BAO measurements (Anderson et al. 2012), together with those from the 6dFGS, SDSS-II and WiggleZ surveys (Beutler et al. 2011; Padmanabhan et al. 2012; Blake et al. 2012) led to a 95% upper limit of 0.44 eV on the sum of the neutrino masses (Hinshaw…”
MethodInfluentialDark Energy Survey year 1 results: Cosmological constraints from galaxy clustering and weak lensing
Abbott, T. M. C., Abdalla, F. B., Alarcon, A., Aleksić, J., Allam, S., Allen, S., Amara, A., Annis, J., Asorey, J., Avila, S., et al. (2018) · Physical Review D · doi:10.1103/physrevd.98.043526 · Cited by 1,213
Wong, K., Suyu, S., Chen, G., Rusu, C., Millon, M., Sluse, D., Bonvin, V., Fassnacht, C., Taubenberger, S., Auger, M., et al. (2019) · Monthly notices of the Royal Astronomical Society · doi:10.1093/mnras/stz3094 · Cited by 966
“…Planck (Planck Collaboration VI 2018b), sometimes including CMB weak lensing (CMBL) results, using the chains provided by the Planck team.4 We can also further combine with baryon acoustic oscillation (BAO) constraints at various redshifts (Beutler et al. 2011; Ross et al. 2015; Alam et al. 2017).”
MethodDESI 2024 VI: cosmological constraints from the measurements of baryon acoustic oscillations
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:10.1088/1475-7516/2025/02/021 · Cited by 1,156
Self-citationBeyond the cosmological standard model
Joyce, A., Jain, B., Khoury, J., & Trodden, M. (2015) · Physics Reports · doi:10.1016/j.physrep.2014.12.002 · Cited by 1,231
Planck 2013 results. XXII. Constraints on inflation
Ade, P. A. R., Aghanim, N., Armitage-Caplan, C., Arnaud, M., Ashdown, M., Atrio-Barandela, F., Aumont, J., Baccigalupi, C., Banday, A. J., Barreiro, R. B., et al. (2014) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201321569 · Cited by 1,539
Early Dark Energy can Resolve the Hubble Tension
Poulin, V., Smith, T. L., Karwal, T., & Kamionkowski, M. (2019) · Physical Review Letters · doi:10.1103/physrevlett.122.221301 · Cited by 1,011
“[22] Florian Beutler, Chris Blake, Matthew Colless, D.”
BackgroundThe Baryon Oscillation Spectroscopic Survey of SDSS-III
Verde, L., Miralda Escudé, J., Cuesta, A. J., & Pérez-Ràfols, I. (2012) · Dipòsit Digital de la Universitat de Barcelona (Universitat de Barcelona) · Cited by 1,201
The WiggleZ Dark Energy Survey: joint measurements of the expansion and growth history at z < 1
Blake, C., Brough, S., Colless, M., Contreras, C., Couch, W., Croom, S., Croton, D., Davis, T. M., Drinkwater, M. J., Forster, K., et al. (2012) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2012.21473.x · Cited by 929
“Some applications to galaxy datasets are presented by Eisenstein et al. (2005), Percival et al. (2010), Beutler et al. (2011), Blake et al. (2011b), Padmanabhan et al. (2012) and Anderson et al. (2012).”
BackgroundMethodSelf-citationBaryon acoustic oscillations in the Lyαforest of BOSS DR11 quasars
Delubac, T., Bautista, J., Busca, N. G., Rich, J., Kirkby, D. P., Bailey, S., Font-Ribera, A., Slosar, A., Lee, K., Pieri, M. M., et al. (2014) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201423969 · Cited by 914
“Other measurements of DV/rd were made at z ∼ 0.1 by the 6dFGRS (Beutler et al., 2011), at (0.4 < z < 0.8) by WiggleZ (Blake et al., 2011a), and, using galaxy clusters, at z ∼ 0.3 by Veropalumbo et al. (2013).”
MethodInfluentialChallenges for Λ CDM: An update
Perivolaropoulos, L., & Skara, F. (2022) · New Astronomy Reviews · doi:10.1016/j.newar.2022.101659 · Cited by 1,130
Anderson, L., Aubourg, É., Bailey, S., Bizyaev, D., Blanton, M. R., Bolton, A. S., Brinkmann, J., Brownstein, J. R., Burden, A., Cuesta, A. J., et al. (2012) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2012.22066.x · Cited by 895
THE SDSS-IV EXTENDED BARYON OSCILLATION SPECTROSCOPIC SURVEY: OVERVIEW AND EARLY DATA
Dawson, K., Kneib, J., Percival, W. J., Alam, S., Albareti, F. D., Anderson, S. F., Armengaud, E., Aubourg, É., Bailey, S., Bautista, J., et al. (2016) · The Astronomical Journal · doi:10.3847/0004-6256/151/2/44 · Cited by 866
“…have been other successful BAO programs (e.g. the 2dF Galaxy Redshift Survey, 6dF Galaxy Survey and WiggleZ Dark Energy Survey; Cole et al. 2005; Beutler et al. 2011; Blake et al. 2011b), we only review BOSS here because it provides a direct demonstration of spectroscopic constraints on…”
MethodSelf-citationAghanim, N., Akrami, Y., Ashdown, M., Aumont, J., Baccigalupi, C., Ballardini, M., Banday, A. J., Barreiro, R. B., Bartolo, N., Basak, S., et al. (2019) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201833886 · Cited by 785
“The joint 68 % and 95 % constraints from CMB lensing with the addition of BAO data (Beutler et al. 2011; Ross et al. 2015; Alam et al. 2017) are shown as the dashed contours, and the constraint from the Planck CMB power-spectrum data is shown for comparison as the solid contours.”
Method2020 global reassessment of the neutrino oscillation picture
de Salas, P. F., Forero, D., Gariazzo, S., Martínez-Miravé, P., Mena, O., Ternes, C. A., Tórtola, M., & Valle, J. W. F. (2021) · Journal of High Energy Physics · doi:10.1007/jhep02(2021)071 · Cited by 769
“We include BAO observations from the 6dF [106], SDSS DR7 Main Galaxy Sample (MGS) [107] and BOSS DR12 [108] galaxy redshift surveys.”
MethodBernal, J. L., Verde, L., & Riess, A. G. (2016) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2016/10/019 · Cited by 748
“J C A P 1 0 ( 2 0 1 6 ) 0 1 9 Survey zeff Parameter Measurement 6dF [33] 0.”
Cosmological implications of baryon acoustic oscillation measurements
Aubourg, É., Bailey, S., Bautista, J., Beutler, F., Bhardwaj, V., Bizyaev, D., Blanton, M. R., Blomqvist, M., Bolton, A. S., Bovy, J., et al. (2015) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.92.123516 · Cited by 743
Self-citationMontePython 3: Boosted MCMC sampler and other features
Brinckmann, T., & Lesgourgues, J. (2019) · Physics of the Dark Universe · doi:10.1016/j.dark.2018.100260 · Cited by 773
“0 SC [43] SDSS DR7: MGS [45] bicep BICEP CMB 1.”
BackgroundPadmanabhan, N., Xu, X., Eisenstein, D. J., Scalzo, R. A., Cuesta, A. J., Mehta, K., & Kazin, E. A. (2012) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2012.21888.x · Cited by 690
“…Padmanabhan et al. 2007; Percival et al. 2007, 2010; Gaztañaga et al. 2009a; Gaztañaga, Cabré & Hui 2009b; Kazin et al. 2010; Reid et al. 2010; Beutler et al. 2011; Sawangwit et al. 2011; Chuang & Wang 2012; Ho et al. 2012; Seo et al. 2012) and current (Hill et al. 2008; Schlegel, White &…”
BackgroundDark Energy Survey Year 1 results: Cosmological constraints from cosmic shear
Troxel, M., MacCrann, N., Zuntz, J., Eifler, T., Krause, E., Dodelson, S., Gruen, D., Blazek, J., Friedrich, O., Samuroff, S., et al. (2017) · Physical Review D · doi:10.1103/physrevd.98.043528 · Cited by 427
Hubble constant hunter’s guide
Knox, L., & Millea, M. (2020) · Physical Review D · doi:10.1103/physrevd.101.043533 · Cited by 638
Baryon acoustic oscillations in the Ly α forest of BOSS quasars
Busca, N. G., Delubac, T., Rich, J., Bailey, S., Font-Ribera, A., Kirkby, D. P., Goff, J.-M. L., Pieri, M. M., Slosar, A., Aubourg, É., et al. (2013) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201220724 · Cited by 631
The Atacama Cosmology Telescope: DR4 maps and cosmological parameters
Aiola, S., Calabrese, E., Maurin, L., Naess, S., Schmitt, B. L., Abitbol, M. H., Addison, G. E., Ade, P. A. R., Alonso, D., Amiri, M., et al. (2020) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2020/12/047 · Cited by 636
Cosmology from cosmic shear power spectra with Subaru Hyper Suprime-Cam first-year data
Hikage, C., Oguri, M., Hamana, T., More, S., Mandelbaum, R., Takada, M., Köhlinger, F., Miyatake, H., Nishizawa, A. J., Aihara, H., et al. (2019) · Publications of the Astronomical Society of Japan · doi:10.1093/pasj/psz010 · Cited by 657
“The BAO dataset includes the measurements of angular diameter distances from the 6dF Galaxy Survey (Beutler et al. 2011), the SDSS DR7 Main Galaxy Sample (Ross et al. 2015), and BOSS LOWZ and CMASS DR12 sample (Alam et al. 2017).”
MethodPlanck2013 results. XX. Cosmology from Sunyaev–Zeldovich cluster counts
Ade, P. A. R., Aghanim, N., Armitage-Caplan, C., Arnaud, M., Ashdown, M., Atrio-Barandela, F., Aumont, J., Baccigalupi, C., Banday, A. J., Barreiro, R. B., et al. (2014) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201321521 · Cited by 620
“In the latter case we adopt the combined likelihood of Hinshaw et al. (2013) and Planck Collaboration XVI (2014), which uses the radial BAO scales observed by 6dFGRS (Beutler et al. 2011), SDSS-DR7-rec and SDSS-DR9rec (Padmanabhan et al. 2012; Anderson et al. 2012), and WiggleZ (Blake et al. 2012).”
MethodPlanck evidence for a closed Universe and a possible crisis for cosmology
Di Valentino, E., Melchiorri, A., & Silk, J. (2019) · Nature Astronomy · doi:10.1038/s41550-019-0906-9 · Cited by 673
The Atacama Cosmology Telescope: DR4 maps and cosmological parameters
Aiola, S., Calabrese, E., Maurin, L., Næss, S., Schmitt, B., Abitbol, M., Addison, G., Ade, P. A. R., Alonso, D., Amiri, M., et al. (2020) · eScholarship (California Digital Library) · Cited by 544
Baumann, D., & McAllister, L. (2015) · Cambridge University Press eBooks · doi:10.1017/cbo9781316105733 · Cited by 621
Snowmass2021—Letter of interest cosmology intertwined II: The hubble constant tension
Di Valentino, E., Anchordoqui, L. A., Akarsu, Ö., Ali-Haimoud, Y., Amendola, L., Arendse, N., Asgari, M., Ballardini, M., Basilakos, S., Battistelli, E., et al. (2021) · Astroparticle Physics · doi:10.1016/j.astropartphys.2021.102605 · Cited by 513
“[6] F.”
New physics in light of the H 0 tension: An alternative view
Vagnozzi, S. (2020) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.102.023518 · Cited by 515
The 6dF Galaxy Survey: z≈ 0 measurements of the growth rate and σ8
Beutler, F., Blake, C., Colless, M., Jones, D. H. P., Staveley‐Smith, L., Poole, G. B., Campbell, L., Parker, Q. A., Saunders, W., & Watson, F. G. (2012) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2012.21136.x · Cited by 509
“This agrees with the findings of Beutler et al. (2011).”
MethodInfluentialSelf-citationAlbareti, F. D., Prieto, C. A., Almeida, A., Anders, F., Anderson, S., Andrews, B. H., Aragón‐Salamanca, A., Argudo-Fernández, M., Armengaud, E., Aubourg, É., et al. (2017) · The Astrophysical Journal Supplement Series · doi:10.3847/1538-4365/aa8992 · Cited by 509
Teleparallel gravity: from theory to cosmology
Bahamonde, S., Dialektopoulos, K. F., Escamilla‐Rivera, C., Farrugia, G., Gakis, V., Hendry, M., Hohmann, M., Said, J. L., Mifsud, J., & Valentino, E. D. (2022) · Reports on Progress in Physics · doi:10.1088/1361-6633/ac9cef · Cited by 668
Dynamical dark energy in light of the latest observations
Zhao, G., Raveri, M., Pogosian, L., Wang, Y., Crittenden, R., Handley, W. J., Percival, W. J., Beutler, F., Brinkmann, J., Chuang, C.-H., et al. (2017) · Nature Astronomy · doi:10.1038/s41550-017-0216-z · Cited by 491
Self-citationAde, P. A. R., Aghanim, N., Arnaud, M., Ashdown, M., Aumont, J., Baccigalupi, C., Banday, A. J., Barreiro, R. B., Bartlett, J. G., Bartolo, N., et al. (2016) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201525833 · Cited by 990
Albareti, F. D., Prieto, C. A., Almeida, A., Anders, F., Anderson, S. F., Andrews, B. H., Aragón‐Salamanca, A., Argudo–Fernández, M., Armengaud, E., Aubourg, É., et al. (2017) · Infoscience (Ecole Polytechnique Fédérale de Lausanne) · doi:10.17863/cam.20755 · Cited by 470
THE 1% CONCORDANCE HUBBLE CONSTANT
Bennett, C. L., Larson, D., Weiland, J. L., & Hinshaw, G. (2014) · The Astrophysical Journal · doi:10.1088/0004-637x/794/2/135 · Cited by 465
The H0 Olympics: A fair ranking of proposed models
Schöneberg, N., Abell'an, G. F., Sanchez, A., Witte, S. J., Poulin, V., & Lesgourgues, J. (2021) · Physics reports · doi:10.1016/j.physrep.2022.07.001 · Cited by 400
“Dbaseline = Planck 2018 (including TTTEEE and lensing) [62] + BAO (including BOSS DR12 [63] + MGS [64] + 6dFGS [65]) + Pantheon [41] ,”
The $H_0$ Olympics: A fair ranking of proposed models
Schöneberg, N., Abellán, G. F., Sánchez, A. P., Witte, S. J., Poulin, V., & Lesgourgues, J. (2021) · arXiv · doi:10.48550/arxiv.2107.10291 · Cited by 463
“Dbaseline = Planck 2018 (including TTTEEE and lensing) [62] + BAO (including BOSS DR12 [63] + MGS [64] + 6dFGS [65]) + Pantheon [41] ,”
Bonvin, V., Courbin, F., Suyu, S. H., Marshall, P. J., Rusu, C. E., Sluse, D., Tewes, M., Wong, K. C., Collett, T., Fassnacht, C. D., et al. (2017) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stw3006 · Cited by 457
“…(Planck Collaboration et al. 2015b, hereafter “CMBL”), with Baryon Acoustic Oscillations surveys at various redshifts (Percival et al. 2010; Beutler et al. 2011; Blake et al. 2011; Anderson et al. 2012; Padmanabhan et al. 2012, hereafter BAO) and with the data of the Joint Lightcurve…”
Testing general relativity in cosmology
Ishak, M. (2019) · Living Reviews in Relativity · doi:10.1007/s41114-018-0017-4 · Cited by 449
Measurement of baryon acoustic oscillation correlations atz = 2.3 with SDSS DR12 Lyα-Forests
Bautista, J., Busca, N. G., Guy, J., Rich, J., Blomqvist, M., Bourboux, H. D. M. D., Pieri, M. M., Font-Ribera, A., Bailey, S., Delubac, T., et al. (2017) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201730533 · Cited by 431
“± 8.) km s−1 Mpc−1 147.33 Mpc rd (31) Figure 17 displays this result along with those of Alam et al. (2016), Beutler et al. (2011), Ross et al. (2015) and Font-Ribera et al. (2014).”
InfluentialPlanck 2015 resultsXV. Gravitational lensing
Ade, P. A. R., Aghanim, N., Arnaud, M., Ashdown, M., Aumont, J., Baccigalupi, C., Banday, A. J., Barreiro, R. B., Bartlett, J. G., Bartolo, N., et al. (2016) · LA Referencia (Red Federada de Repositorios Institucionales de Publicaciones Científicas) · doi:10.1051/0004-6361/201525941 · Cited by 284
Reid, B., Samushia, L., White, M. J., Percival, W. J., Manera, M., Padmanabhan, N., Ross, A. J., Sánchez, A. G., Bailey, S., Bizyaev, D., et al. (2012) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2012.21779.x · Cited by 425
“…al. 2007; Padmanabhan et al. 2007; Percival et al. 2007, 2010; Okumura et al. 2008; Gaztanaga, Cabre & Hui 2009; Kazin et al. 2010; Reid et al. 2010b; Beutler et al. 2011; Blake et al. 2011a) have revealed that the expansion of the Universe is accelerating; either the energy density of the…”
BackgroundCan interacting dark energy solve the H0 tension?
Valentino, E. D., MELCHIORRI, A., & Mena, O. (2017) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.96.043503 · Cited by 419
Ata, M., Baumgarten, F., Bautista, J., Beutler, F., Bizyaev, D., Blanton, M. R., Blazek, J., Bolton, A. S., Brinkmann, J., Brownstein, J. R., et al. (2017) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stx2630 · Cited by 415
“…Sloan Digital Sky Survey (SDSS) I and II (e.g. Eisenstein et al. 2005; Percival et al. 2010; Ross et al. 2015), the 2-degree Field Galaxy Redshift Survey (2dFGRS) (Percival et al. 2001; Cole et al. 2005), WiggleZ (Blake et al. 2011), and the 6-deg Field Galaxy Survey (6dFGS) (Beutler et al. 2011).”
BackgroundSelf-citationUnveiling ν secrets with cosmological data: Neutrino masses and mass hierarchy
Vagnozzi, S., Giusarma, E., Mena, O., Katherine Freese, B., Gerbino, M., Ho, S., & Lattanzi, M. (2017) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.96.123503 · Cited by 411
THE ATACAMA COSMOLOGY TELESCOPE: COSMOLOGICAL PARAMETERS FROM THE 2008 POWER SPECTRUM
Dunkley, J., Hložek, R., Sievers, J. L., Acquaviva, V., Ade, P. A. R., Aguirre, P., Amiri, M., Appel, J. W., Barrientos, L. F., Battistelli, E. S., et al. (2011) · The Astrophysical Journal · doi:10.1088/0004-637x/739/1/52 · Cited by 428
Nonminimal dark sector physics and cosmological tensions
Valentino, E. D., MELCHIORRI, A., Mena, O., & Vagnozzi, S. (2020) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.101.063502 · Cited by 389
Bourboux, H. D. M. D., Rich, J., Font-Ribera, A., Agathe, V. D. S., Farr, J., Etourneau, T., Goff, J.-M. L., Cuceu, A., Balland, C., Bautista, J., et al. (2020) · The Astrophysical Journal · doi:10.3847/1538-4357/abb085 · Cited by 398
“At redshifts z2 the BAO scale has been studied using discrete tracers such as galaxies (Percival et al. 2007, 2010; Beutler et al. 2011; Blake et al. 2011; Anderson et al. 2012, 2014a, 2014b; Chuang & Wang 2012; Mehta et al. 2012; Padmanabhan et al. 2012; Xu et al. 2013; Ross et al. 2015; Alam et…”
MethodCapozzıello, S., D’Agostino, R., & Luongo, O. (2019) · International Journal of Modern Physics D · doi:10.1142/s0218271819300167 · Cited by 427
The WiggleZ Dark Energy Survey: joint measurements of the expansion and growth history at z 1Preprint
Blake, C., Brough, S., Colless, M., Contreras, C., Couch, W. J., Croom, S. M., Croton, D., Davis, T. M., Drinkwater, M. J., Förster, K., et al. (2024) · doi:10.25916/sut.26242559.v1 · Cited by 392
Self-citationAbbott, T., Abdalla, F., Ávila, S., Banerji, M., Baxter, E., Bechtol, K., Becker, M., Bertin, E., Blazek, J., Bridle, S., et al. (2018) · Physical Review D · doi:10.1103/physrevd.99.123505 · Cited by 149
On the Hubble Constant Tension in the SNe Ia Pantheon Sample
Dainotti, M. G., Simone, B. D., Schiavone, T., Montani, G., Rinaldi, E., & Lambiase, G. (2021) · The Astrophysical Journal · doi:10.3847/1538-4357/abeb73 · Cited by 377
Valentino, E. D., MELCHIORRI, A., Mena, O., & Vagnozzi, S. (2020) · Physics of the Dark Universe · doi:10.1016/j.dark.2020.100666 · Cited by 384
Ade, P. A. R., Aghanim, N., Arnaud, M., Ashdown, M., Aumont, J., Baccigalupi, C., Banday, A. J., Barreiro, R. B., Bartolo, N., Battaner, E., et al. (2016) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201525814 · Cited by 814
“2011) and 6dF Galaxy Survey (6dFGS) (Beutler et al. 2012), together with CFHTLenS WL. Baker et al. (2014) provided forecasts on μ0−1 and Σ0 − 1 for a future experiment that combines galaxy clustering and tomographic weak lensing measurements. The amplitude of departures from the standard values was parameterized as in…”
InfluentialThe Atacama Cosmology Telescope: DR6 Gravitational Lensing Map and Cosmological Parameters
Madhavacheril, M. S., Qu, F. J., Sherwin, B. D., MacCrann, N., Li, Y., Abril-Cabezas, I., Ade, P. A. R., Aiola, S., Alford, T., Amiri, M., et al. (2024) · The Astrophysical Journal · doi:10.3847/1538-4357/acff5f · Cited by 366
“We combine the power spectrum of the fluctuations in this map with measure- ments of the baryon acoustic oscillations (BAO) measured by 6dF (Beutler et al. 2011) and the Sloan Digital Sky Survey (SDSS; Strauss et al. 2002; Eisenstein et al. 2011; Dawson et al. 2013) to obtain one of the most…”
MethodCurvature tension: Evidence for a closed Universe
Handley, W. (2021) · Physical Review D · doi:10.1103/physrevd.103.l041301 · Cited by 377
“[15] Florian Beutler, Chris Blake, Matthew Colless, D.”
Reconciling Planck with the local value of H 0 in extended parameter space
Valentino, E. D., MELCHIORRI, A., & Silk, J. I. (2016) · Physics Letters B · doi:10.1016/j.physletb.2016.08.043 · Cited by 359
Kazin, E. A., Koda, J., Blake, C., Padmanabhan, N., Brough, S., Colless, M., Contreras, C., Couch, W. J., Croom, S. M., Croton, D., et al. (2014) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stu778 · Cited by 358
“In the right-hand panel, we compare with two results from the SDSS-II (cyan star, 0.2 < z < 0.44; Padmanabhan et al. 2012) and SDSS-III (magenta triangles 0.2 < z < 0.43 0.43 < z < 0.7; Anderson et al. 2014a), as well as the result obtained by the 6dFGS ( z ∼ 0.1; Beutler et al. 2011).”
InfluentialSelf-citationBeutler, F., Seo, H., Saito, S., Chuang, C.-H., Cuesta, A. J., Eisenstein, D. J., Gil-Marín, H., Grieb, J. N., Hand, N., Kitaura, F.-S., et al. (2016) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stw3298 · Cited by 354
“The wide angle effect has been shown to be negligible compared to the sample variance for surveys such as BOSS (Beutler et al. 2011, 2012; Samushia, Percival & Raccanelli 2011; Yoo & Seljak 2015).”
BackgroundSelf-citationThe Atacama Cosmology Telescope: cosmological parameters from three seasons of data
Sievers, J. L., Hložek, R., Nolta, M. R., Acquaviva, V., Addison, G. E., Ade, P. A. R., Aguirre, P., Amiri, M., Appel, J. W., Barrientos, L. F., et al. (2013) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2013/10/060 · Cited by 352
“The solid curves are for ACT plus WMAP7, and the dashed lines add priors from measurements of the baryon acoustic peak [6, 20, 142] and a direct measurement of H0 [153].”
MethodTHE PHENOMENOLOGY OF RIGHT HANDED NEUTRINOS
Drewes, M. (2013) · International Journal of Modern Physics E · doi:10.1142/s0218301313300191 · Cited by 392
Tale of stable interacting dark energy, observational signatures, and the H0 tension
Yang, W., Pan, S., Valentino, E. D., Nunes, R. C., Vagnozzi, S., & Mota, D. F. (2018) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2018/09/019 · Cited by 345
“106) [111], (ii) the Main Galaxy Sample of Data Release 7 of the Sloan Digital Sky Survey (SDSS-MGS) (zeff = 0.”
BackgroundNeutrino puzzle: Anomalies, interactions, and cosmological tensions
Kreisch, C. D., Cyr-Racine, F.-Y., & Doré, O. (2020) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.101.123505 · Cited by 345
Rest, A., Scolnic, D. M., Foley, R. J., Huber, M. E., Chornock, R., Narayan, G., Tonry, J. L., Berger, E., Soderberg, A., Stubbs, C. W., et al. (2014) · The Astrophysical Journal · doi:10.1088/0004-637x/795/1/44 · Cited by 340
Oscillating scalar fields and the Hubble tension: A resolution with novel signatures
Smith, T. L., Poulin, V., & Amin, M. A. (2020) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.101.063523 · Cited by 338
Global constraints on absolute neutrino masses and their ordering
Capozzi, F., Valentino, E. D., Lisi, E., Marrone, A., MELCHIORRI, A., & Palazzo, A. (2017) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.95.096014 · Cited by 336
“(iv) The baryon acoustic oscillation measurements from 6dFGS [88], SDSS-MGS [89], BOSSLOWZ [90], and CMASS-DR11 [90] surveys as done in [19].”
MethodDark energy two decades after: observables, probes, consistency tests
Dragan Huterer, A., & Shafer, D. L. (2017) · Reports on Progress in Physics · doi:10.1088/1361-6633/aa997e · Cited by 328
Yu, H.-B., Ratra, B., & Wang, F.-Y. (2017) · The Astrophysical Journal · doi:10.3847/1538-4357/aab0a2 · Cited by 298
Valentino, E. D., Said, J. L., Riess, A. G., Pollo, A., Poulin, V., Gómez-Valent, A., Weltman, A., Palmese, A., Huang, C. D., van de Bruck, C., et al. (2025) · Physics of the Dark Universe · doi:10.1016/j.dark.2025.101965 · Cited by 590
Self-citationBeutler, F., Saito, S., Seo, H., Brinkmann, J., Dawson, K., Eisenstein, D. J., Font-Ribera, A., Ho, S., McBride, C. K., Montesano, F., et al. (2014) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stu1051 · Cited by 341
“It has been shown, however, that the local plane-parallel approximation is a very good approximation for most galaxy samples even when they cover a large fraction of the sky (Beutler et al. 2011; Samushia, Percival & Raccanelli 2012; Yoo & Seljak 2013).”
BackgroundSelf-citationStochastic gravitational wave backgrounds
Christensen, N. L. (2018) · Reports on Progress in Physics · doi:10.1088/1361-6633/aae6b5 · Cited by 376
Kitaura, F.-S., Rodríguez-Torres, S. A., Chuang, C.-H., Zhao, C., Prada, F., Gil-Marín, H., Guo, H., Yepes, G., Klypin, A. A., Scóccola, C. G., et al. (2016) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stv2826 · Cited by 320
“…of large surveys (Percival et al. 2001; Cole et al. 2005) was done based on lognormal realizations (see also Percival, Verde & Peacock 2004; Beutler et al. 2011), which match the two-point statistics by construction (Coles & Jones 1991), although their three-point statistics is very…”
BackgroundSelf-citationEarly dark energy does not restore cosmological concordance
Hill, J. C., McDonough, E., Toomey, M. W., & Alexander, S. (2020) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.102.043507 · Cited by 316
“…probes the low-redshift universe, we include: BAO: Measurements from the SDSS DR7 main galaxy sample (Ross et al. (2015)) and the 6dF galaxy survey (Beutler et al. (2011)) at z = 0.15 and z = 0.106, respectively, as well as from the SDSS BOSS DR12 (Alam et al. (2017)) optimally combined LOWZ and…”
MethodInfluentialBautista, J., Paviot, R., Vargas-Magaña, M., de la Torre, S., Fromenteau, S., Gil-Marín, H., Ross, A. J., Burtin, E., Dawson, K., Hou, J., et al. (2020) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/staa2800 · Cited by 313
Weighing the giants – IV. Cosmology and neutrino mass
Mantz, A. B., von der Linden, A., Allen, S. W., Applegate, D., Kelly, P. L., Morris, R. G., Rapetti, D., Schmidt, R. W., Adhikari, S., Allen, M. T., et al. (2014) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stu2096 · Cited by 315
“…type Ia supernovae (Suzuki et al. 2012) and baryon acoustic oscillation (BAO) data from the combination of results from the 6-degree Field Galaxy Survey (6dF; z = 0.106; Beutler et al. 2011) and the Sloan Digital Sky Survey (SDSS, z = 0.35 and 0.57; Padmanabhan et al. 2012; Anderson et al. 2014).”
BackgroundInfluentialNeutrino masses and cosmology with Lyman-alpha forest power spectrum
Palanque‐Delabrouille, N., Yèche, C., Baur, J., Magneville, C., Rossi, G., Julien Lesgourgues, A., Borde, A., Burtin, E., LeGoff, J.-M., Rich, J., et al. (2015) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2015/11/011 · Cited by 304
“Finally, we occasionally combine CMB data with measurements of the BAO scale by 6dFGS [17], SDSS main galaxy sample [18], BOSS-LOWZ [19] and CMASS-DR11 [19].”
MethodCMB lensing from Planck PR4 maps
Carron, J., Mirmelstein, M., & Lewis, A. (2022) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2022/09/039 · Cited by 301
“The BAO likelihoods for PR4 use the 6dF Galaxy Survey measurements [43], the SDSS Data Release (DR) 7 measurements [44] and the angular and radial DR12+DR16 LRG data from eBOSS [45], with the exception of the fourth entry, which uses the same BAO likelihoods and priors of PR3.”
MethodCosmological implications of ultralight axionlike fields
Poulin, V., Smith, T. L., Grin, D., Karwal, T., & Kamionkowski, M. (2018) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.98.083525 · Cited by 294
Flavor structures of charged fermions and massive neutrinos
Xing, Z. (2020) · Physics Reports · doi:10.1016/j.physrep.2020.02.001 · Cited by 339
“The final full-mission Planck measurements of the CMB anisotropies [87], combined with the BAO measurements [335, 336, 337], strongly support the”
Method
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
About these checks
Registry, retraction, Cites and statistics results are computed, not judged, with one exception: a printed reference that no index lists is read once by a model before it counts as a citation error. Claims are extracted by a model and kept only when their quote appears verbatim in the text; each cited source is then checked, with a model’s help, for whether it says what the claim relies on. Those verdicts can be wrong — read the claim’s quote and the cited source before relying on one.
Statistics and arithmetic are recomputed, not judged.
Confidence bands are shown only for fields calibrated on our annotated test set. None is calibrated yet, so no band is shown.
What counts as a claim ›How we measure confidence ›How we check this ›
Are you an author, or do you see a problem with this page? Request a review
