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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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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
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“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
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“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
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BackgroundMethodInfluentialFinal Results from the Hubble Space Telescope Key Project to Measure the Hubble Constant
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- Arnalte-Mur, 2011, MNRAS
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Items 301–400 of 1,006
Scalar-tensor theories of gravity, neutrino physics, and the H0 tension
Ballardini, M., Braglia, M., Finelli, F., Paoletti, D., Starobinsky, A. A., & Umiltà, C. (2020) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2020/10/044 · Cited by 133
“61 [116–118], in combination with measure from 6dF [39] at zeff = 0.”
BackgroundRedshift-space distortions in f(R) gravity
Jennings, E., Baugh, C. M., Li, B., Zhao, G.-B., & Koyama, K. (2012) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2012.21567.x · Cited by 127
Cuesta, A. J., Verde, L., Riess, A. G., & Jiménez, R. (2015) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stv261 · Cited by 113
“C O precision over the redshift range from z = 0.1 to z > 1 (see e.g., Anderson et al. 2014; Tojeiro et al. 2014; FontRibera et al. 2014; Delubac et al. 2015; Beutler et al. 2011; Ross et al. 2014; Kazin et al. 2014).”
BackgroundMethodInfluentialPseudoscalar—sterile neutrino interactions: reconciling the cosmos with neutrino oscillations
Archidiacono, M., Gariazzo, S., Carlo Giunti, A., Hannestad, S., Hansen, R. S. L., Marco Laveder, B., & Tram, T. (2016) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2016/08/067 · Cited by 113
“75 Km s−1 Mpc−1 [8] (HST) and Baryonic Acoustic Oscillations (BAO) from a list of different experiments, that probe different redshifts: 6dFGS [46], SDSS-MGS [47], and from the LOWZ [48] and CMASS [49] DR11 results from the SDSS BOSS experiment.”
ResultRyan, J., Chen, Y., & Ratra, B. (2019) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stz1966 · Cited by 113
Cosmological constraints from unWISE and Planck CMB lensing tomography
Krolewski, A., Ferraro, S., & White, M. J. (2021) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2021/12/028 · Cited by 113
Exploring Vainshtein mechanism on adaptively refined meshes
Li, B., Zhao, G., & Koyama, K. (2013) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2013/05/023 · Cited by 113
Decaying dark matter and the tension in σ8
Enqvist, K., Nadathur, S., Sekiguchi, T., & Takahashi, T. (2015) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2015/09/067 · Cited by 112
Quantifying tensions in cosmological parameters: Interpreting the DES evidence ratio
Handley, W. J., & Lemos, P. (2019) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.100.043504 · Cited by 112
“[67] Florian Beutler, Chris Blake, Matthew Colless, D.”
MethodUpdated constraints on massive neutrino self-interactions from cosmology in light of the H 0 tension
Choudhury, S. R., Hannestad, S., & Tram, T. (2021) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2021/03/084 · Cited by 112
“J C A P 0 3 ( 2 0 2 1 ) 0 8 4 In addition to the primary data set, we use an auxiliary dataset combination denoted by EXT which consists of Planck 2018 CMB lensing [43], BAO and RSD measurements from SDSS-III BOSS DR12 [31], additional BAO measurements from MGS [32] and 6dFGS [33], and SNe Ia luminosity distance measu…”
MethodResultFuture Cosmological Constraints From Fast Radio Bursts
Walters, A., Weltman, A., Gaensler, B. M., Ma, Y.-Z., & Witzemann, A. (2018) · The Astrophysical Journal · doi:10.3847/1538-4357/aaaf6b · Cited by 111
“…anisotropies (Hinshaw et al. 2013; Planck Collaboration et al. 2016a, 2016b), baryon acoustic oscillation (BAO) wiggles in the galaxy power spectrum (Beutler et al. 2011; Anderson et al. 2014; Ross et al. 2015), luminosity distance–redshift relation of TypeIa supernovae (SNIa; Riess et al. 2004,…”
BackgroundCarter, P., Beutler, F., Percival, W. J., Blake, C., Koda, J., & Ross, A. J. (2018) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/sty2405 · Cited by 111
“Subsequently the BAO peak has been detected in later SDSS data releases (Kazin et al. 2010; Percival et al. 2010), 6dFGS (Beutler et al. 2011), WiggleZ (Blake et al. 2011), BOSS (LOWZ and CMASS; Alam et al. 2017), eBOSS luminous red galaxies (LRGs) (Bautista et al. 2017) and quasars (QSOs; Ata et…”
BackgroundMethodResultInfluentialSelf-citationImplications for the Hubble tension from the ages of the oldest astrophysical objects
Vagnozzi, S., Pacucci, F., & Loeb, A. (2022) · Journal of High Energy Astrophysics · doi:10.1016/j.jheap.2022.07.004 · Cited by 116
White, M. J., Zhou, R., DeRose, J., Ferraro, S., Chen, S.-F., Kokron, N., Bailey, S., Brooks, D., García-Bellido, J., Guy, J., et al. (2022) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2022/02/007 · Cited by 110
Three thermodynamically based parametrizations of the deceleration parameter
del Campo, S., Duran, I., Herrera, R., & Pavón, D. (2012) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.86.083509 · Cited by 109
Bocquet, S., Dietrich, J. P., Schrabback, T., Bleem, L. E., Klein, M., Allen, S. W., Applegate, D., Ashby, M. L. N., Bautz, M. W., Bayliss, M. B., et al. (2019) · The Astrophysical Journal · doi:10.3847/1538-4357/ab1f10 · Cited by 394
“We use angular diameter distances as probed by baryon acoustic oscillations (BAOs) by the 6dF Galaxy Survey (Beutler et al. 2011), the SDSS Data Release7 Main Galaxy Sample (Ross et al. 2015), and the BOSS Data Release12 (Alam et al. 2017).”
MethodRelic neutrinos, thermal axions, and cosmology in early 2014
Giusarma, E., Valentino, E. D., Lattanzi, M., MELCHIORRI, A., & Mena, O. (2014) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.90.043507 · Cited by 108
Constraining dark matter late-time energy injection: decays and p-wave annihilations
Diamanti, R., Lopez-Honorez, L., Mena, O., Palomares-Ruiz, S., & Vincent, A. C. (2014) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2014/02/017 · Cited by 108
“In addition to CMB measurements, we include a prior on the Hubble constant H0 from the HST [44] and BAO measurements from a number of surveys [45–48].”
MethodResultInfluentialCosmological Constraints from Multiple Probes in the Dark Energy Survey
Abbott, T. M. C., Alarcon, A., Allam, S., Andersen, P., Andrade-Oliveira, F., Annis, J. T., Asorey, J., Avila, S., Bacon, D., Banik, N., et al. (2019) · Physical Review Letters · doi:10.1103/physrevlett.122.171301 · Cited by 108
Sánchez, A. G., Kazin, E., Beutler, F., Chuang, C., Cuesta, A., Eisenstein, D., Manera, M., Montesano, F., Nichol, B., Padmanabhan, N., et al. (2013) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stt799 · Cited by 86
“(4) We use the results of Beutler et al. (2011), who obtained an estimate of DV(z = 0.106)/rs = 0.336 ± 0.015 from the large-scale correlation function of the 6dF Galaxy Survey (6dFGS, Jones et al. 2009), and the 2% distance measurement of DV(z = 0.35)/rs = 8.88 ± 0.17 obtained by Padmanabhan et…”
BackgroundMethodInfluentialSelf-citationCosmological axion and neutrino mass constraints from Planck 2015 temperature and polarization data
Valentino, E. D., Giusarma, E., Lattanzi, M., Mena, O., MELCHIORRI, A., & Silk, J. I. (2015) · Physics Letters B · doi:10.1016/j.physletb.2015.11.025 · Cited by 107
The Mira-Titan Universe. III. Emulation of the Halo Mass Function
Bocquet, S., Heitmann, K., Habib, S., Lawrence, E., Uram, T. D., Frontiere, N., Pope, A., & Finkel, H. (2020) · The Astrophysical Journal · doi:10.3847/1538-4357/abac5c · Cited by 107
“…1 also shows current cosmological constraints from Planck TTTEEE+lowl+lowE (Planck Collaboration et al. 2018), Baryon Acoustic Oscillations (BAO, Beutler et al. 2011; Ross et al. 2015; Alam et al. 2017), and the Pantheon supernova sample (Scolnic et al. 2018). particle masses vary between 7.23×…”
BackgroundInfluentialEarly recombination as a solution to the H0 tension
Sekiguchi, T., & Takahashi, T. (2021) · Physical Review D · doi:10.1103/physrevd.103.083507 · Cited by 105
Observational constraints on Hubble constant and deceleration parameter in power-law cosmology
Kumar, S. (2012) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2012.20810.x · Cited by 106
“WMAP seven-year results gave an estimate of H0 = 71.0 ± 2.5 km s −1 Mpc−1 based on WMAP data alone, and an estimate of H0 = 70.4 +1.3 −1.4 km s −1 Mpc−1 based on WMAP data with Gaussian priors corresponding to earlier estimates from other studies (Jarosik et al. 2011).”
MethodInfluentialPlanck constraints on single-field inflation
Tsujikawa, S., Ohashi, J., Kuroyanagi, S., & Felice, A. D. (2013) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.88.023529 · Cited by 105
Park, C., & Ratra, B. (2019) · The Astrophysical Journal · doi:10.3847/1538-4357/ab3641 · Cited by 105
“We use the recent, more reliable BAO distance measurements from the 6dF Galaxy Survey (6dFGS) (Beutler et al. 2011), the Sloan Digital Sky Survey (SDSS) Data Release 7 (DR7) main galaxy sample (MGS) (Ross et al. 2015), the Baryon Oscillation Spectroscopic Survey (BOSS) DR12 galaxies (Alam et al.…”
MethodInfluentialRyan, J., Doshi, S., & Ratra, B. (2018) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/sty1922 · Cited by 105
Interacting radiation after Planck and its implications for the Hubble tension
Blinov, N., & Marques-Tavares, G. (2020) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2020/09/029 · Cited by 105
Beyond six parameters: Extending ΛCDM
Valentino, E. D., MELCHIORRI, A., & Silk, J. I. (2015) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.92.121302 · Cited by 104
Listening to the sound of dark sector interactions with gravitational wave standard sirens
Yang, W., Vagnozzi, S., Valentino, E. D., Nunes, R. C., Pan, S., & Mota, D. F. (2019) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2019/07/037 · Cited by 104
“[193] F. Beutler et al., The 6dF Galaxy Survey: Baryon Acoustic Oscillations and the Local Hubble Constant, Mon.”
MethodA new interacting two-fluid model and its consequences
Sharov, G. S., Bhattacharya, S., Pan, S., Nunes, R. C., & Chakraborty, S. (2016) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stw3358 · Cited by 102
Gómez-Valent, A., & Solà, J. (2018) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/sty1028 · Cited by 102
“…(Howlett et al. 2017), the LSS data point from (Granett et al. 2015) by those from (Pezzota et al. 2017), the BAO data at z = 0.106 from the 6dFGS (Beutler et al. 2011) and at z = 0.15 from SDSS DR7 (Ross et al. 2015) by their combined value at zeff = 0.122 (Carter et al. 2018), the BAO Lyα…”
MethodInfluentialChudaykin, A., Dolgikh, K. A., & Ivanov, M. M. (2021) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.103.023507 · Cited by 102
Abbott, T. M. C., Aguena, M., Allam, S., Amon, A., Andrade-Oliveira, F., Asorey, J., Avila, S., Bernstein, G. M., Bertin, E., Brandao-Souza, A., et al. (2022) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.105.043512 · Cited by 102
Physical effects involved in the measurements of neutrino masses with future cosmological data
Archidiacono, M., Brinckmann, T., Julien Lesgourgues, A., & Poulin, V. (2017) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2017/02/052 · Cited by 101
“Gray error bars refer to the current BAO measurements: from left to right 6dFGRS [15], SDSS MGS [70], LOW-Z, C-MASS [7].”
BackgroundSimulating the quartic Galileon gravity model on adaptively refined meshes
Li, B., Barreira, A., Baugh, C. M., Hellwing, W. A., Koyama, K., Pascoli, S., & Zhao, G. (2013) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2013/11/012 · Cited by 100
Zumalacárregui, M. (2020) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.102.023523 · Cited by 99
Addendum to “Global constraints on absolute neutrino masses and their ordering”
Capozzi, F., Valentino, E. D., Lisi, E., Marrone, A., MELCHIORRI, A., & Palazzo, A. (2020) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.101.116013 · Cited by 100
Evidence for Emergent Dark Energy
Li, X., & Shafieloo, A. (2020) · The Astrophysical Journal · doi:10.3847/1538-4357/abb3d0 · Cited by 100
Self-interacting neutrinos, the Hubble parameter tension, and the cosmic microwave background
Brinckmann, T., Chang, J. H., & Loverde, M. (2021) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.104.063523 · Cited by 103
Cosmokinetics: a joint analysis of standard candles, rulers and cosmic clocks
Nair, R., Jhingan, S., & Jain, D. (2012) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2012/01/018 · Cited by 99
de la Torre, S., Jullo, E., Giocoli, C., Pezzotta, A., Bel, J., Granett, B. R., Guzzo, L., Garilli, B., Scodeggio, M., Bolzonella, M., et al. (2017) · Astronomy & Astrophysics · doi:10.1051/0004-6361/201630276 · Cited by 99
“…statistics of the galaxy distribution and its features (e.g. Peacock et al. 2001; Cole et al. 2005; Tegmark et al. 2004; Eisenstein et al. 2005; Guzzo et al. 2008; Percival et al. 2010; Beutler et al. 2011; Blake et al. 2012; Anderson et al. 2014; Alam et al. 2017, and references therein).”
BackgroundPacif, S. K. J. (2020) · The European Physical Journal Plus · doi:10.1140/epjp/s13360-020-00769-y · Cited by 104
Jee, M. J., Tyson, J. A., Hilbert, S., Schneider, M. D., Schmidt, S., & Wittman, D. (2016) · The Astrophysical Journal · doi:10.3847/0004-637x/824/2/77 · Cited by 98
“We combine the Baryonic Acoustic Oscillation (BAO) results published by Anderson et al. (2012), Padmanabhan et al. (2012), Beutler et al. (2011), and Blake et al. (2012).”
MethodCosmological viable models in f ( T , B ) theory as solutions to the H 0 tension
Escamilla‐Rivera, C., & Said, J. L. (2020) · Classical and Quantum Gravity · doi:10.1088/1361-6382/ab939c · Cited by 109
Field theoretic interpretations of interacting dark energy scenarios and recent observations
Pan, S., Sharov, G. S., & Yang, W. (2020) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.101.103533 · Cited by 98
“We use the latest cosmic microwave background observations from Planck 2018 [85, 86] and baryon acoustic oscillations distance measurements [87, 88, 89].”
MethodNon-linear interacting cosmological models after Planck 2018 legacy release and the H0 tension
Pan, S., Yang, W., & Paliathanasis, A. (2020) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/staa213 · Cited by 98
“tions (BAO) distance measurements from the experiments 6dFGS [71], SDDS MGS [72], and BOSS DR12 [73].”
Method2021-H 0 odyssey: closed, phantom and interacting dark energy cosmologies
Yang, W., Pan, S., Valentino, E. D., Mena, O., & MELCHIORRI, A. (2021) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2021/10/008 · Cited by 98
Impact of Destination Image Formation on Tourist Trust: Mediating Role of Tourist Satisfaction
Jebbouri, A., Zhang, H., Imran, Z., Iqbal, J., & Bouchiba, N. (2022) · Frontiers in Psychology · doi:10.3389/fpsyg.2022.845538 · Cited by 157
“satisfaction, willingness to return, commitment, and loyalty (Beutler et al., 2011).”
BackgroundHints of early dark energy in Planck , SPT, and ACT data: New physics or systematics?
Smith, T. L., Lucca, M., Poulin, V., Abellán, G. F., Balkenhol, L., Benabed, K., Galli, S., & Murgia, R. (2022) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.106.043526 · Cited by 99
“[51] Florian Beutler, Chris Blake, Matthew Colless, D.”
Spherical collapse in Galileon gravity: fifth force solutions, halo mass function and halo bias
Barreira, A., Li, B., Baugh, C. M., & Pascoli, S. (2013) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2013/11/056 · Cited by 97
“We also show the value of χ 2 = −2logP (where P is the posterior probability obtained from the data from the WMAP 9yr results [1], the SNLS 3yr sample [3] and the BAO measurements from the 6dF Galaxy Survey [8], from the SDSS DR7 [7] and from the SDSS-III BOSS [11]), the Galileon field time derivative at zi, the age o…”
MethodYang, W., Pan, S., & Mota, D. F. (2017) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.96.123508 · Cited by 97
w−M phantom transition at zt<0.1 as a resolution of the Hubble tension
Alestas, G., Kazantzidis, L., & Perivolaropoulos, L. (2021) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.103.083517 · Cited by 97
“[68] Florian Beutler, Chris Blake, Matthew Colless, D.”
Accelerating f(T) gravity models constrained by recent cosmological data
Cardone, V. F., Radicella, N., & Camera, S. (2012) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.85.124007 · Cited by 96
Constraints on dark matter annihilation from CMB observations before Planck
Lopez-Honorez, L., Mena, O., Palomares-Ruiz, S., & Vincent, A. C. (2013) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2013/07/046 · Cited by 96
“106 from the 6dF Galaxy Survey (6dFGS) [103] and the BAO measurements from the WiggleZ Survey at z = 0.”
MethodMeasuring dark energy with theEiso–Epcorrelation of gamma-ray bursts using model-independent methods
Wang, J. S., Wang, F. Y., Cheng, K. S., & Dai, Z. G. (2015) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201526485 · Cited by 96
“We also compare our results to the current precise measurements, such as the results from Planck+WMAP (Planck Collaboration XVI 2013), BAO (Beutler et al. 2011; Anderson et al. 2014; Kazin et al. 2014; Ross et al. 2015), and SNe Ia (Conley et al. 2011; Suzuki et al. 2012).”
ResultHow the dark energy can reconcile Planck with local determination of the Hubble constant
Huang, Q.-G., & Wang, K. (2016) · The European Physical Journal C · doi:10.1140/epjc/s10052-016-4352-x · Cited by 96
Cosmology and dark energy from joint gravitational wave-GRB observations
Belgacem, E., Dirian, Y., Foffa, S., Howell, E. J., Maggiore, M., & Regimbau, T. (2019) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2019/08/015 · Cited by 96
Li, Y.-H., & Zhang, X. (2014) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.89.083009 · Cited by 97
Marin, F. A., Blake, C., Poole, G. B., McBride, C. K., Brough, S., Colless, M., Contreras, C., Couch, W. J., Croton, D., Croom, S. M., et al. (2013) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stt520 · Cited by 95
“…we use; an example is the cosmological constraints from baryon acoustic oscillation (BAO) measurements (Cole et al. 2005; Eisenstein et al. 2005; Beutler et al. 2011; Blake et al. 2011a; Sánchez et al. 2012) where parameters such as the cosmic distance scale and the Hubble expansion rate H(z)…”
MethodSelf-citationIs exponential gravity a viable description for the whole cosmological history?
Odintsov, S. D., Gómez, D. S.-C., & Sharov, G. S. (2017) · The European Physical Journal C · doi:10.1140/epjc/s10052-017-5419-z · Cited by 95
Yang, W., Pan, S., Nunes, R. C., & Mota, D. F. (2020) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2020/04/008 · Cited by 95
Constraints on primordial gravitational waves from the cosmic microwave background
Clarke, T. J., Copeland, E. J., & Moss, A. (2020) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2020/10/002 · Cited by 98
Constraining Dark Matter-Dark Radiation interactions with CMB, BAO, and Lyman-α
Archidiacono, M., Hooper, D. C., Murgia, R., Bohr, S., Julien Lesgourgues, A., & Viel, M. (2019) · RWTH Publications (RWTH Aachen) · Cited by 95
Relieving the H 0 tension with a new interacting dark energy model
Gao, L.-Y., Zhao, Z.-W., Xue, S.-S., & Zhang, X. (2021) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2021/07/005 · Cited by 93
Cosmological constraints on dark matter interactions with ordinary matter
Buen-Abad, M. A., Essig, R., McKeen, D., & Zhong, Y.-M. (2022) · Physics Reports · doi:10.1016/j.physrep.2022.02.006 · Cited by 95
Improving measurements of H(z) and DA (z) by analysing clustering anisotropies
Kazin, E. A., Sánchez, A. G., & Blanton, M. R. (2011) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2011.19962.x · Cited by 95
Zhao, M.-M., He, D.-Z., Zhang, J., & Zhang, X. (2017) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.96.043520 · Cited by 93
Planck 2015 Constraints on the Non-flat ΛCDM Inflation Model
Ooba, J., Ratra, B., & Sugiyama, N. (2018) · The Astrophysical Journal · doi:10.3847/1538-4357/aad633 · Cited by 93
Wang, L.-F., Zhang, X.-N., Zhang, X., & Zhang, X. (2018) · Physics Letters B · doi:10.1016/j.physletb.2018.05.027 · Cited by 92
Reconciling H0 tension in a six parameter space?
Pan, S., Yang, W., Valentino, E. D., Shafieloo, A., & Chakraborty, S. (2020) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2020/06/062 · Cited by 95
“Baryon acoustic oscillation (BAO) distance measurements: we use 6dFGS [4], SDSSMGS [5], and BOSS DR12 [6] surveys, as considered by the Planck collaboration [3].”
MethodPhysical effects involved in the measurements of neutrino masses with future cosmological data
Archidiacono, M., Brinckmann, T., Julien Lesgourgues, A., & Poulin, V. (2016) · CERN Document Server (European Organization for Nuclear Research) · Cited by 92
Abbott, T. M. C., Allam, S., Andersen, P., Angus, C. R., Asorey, J., Avelino, A., Avila, S., Bassett, B. A., Bechtol, K., Bernstein, G. M., et al. (2019) · Sussex Research Online (University of Sussex) · doi:10.17863/cam.41220 · Cited by 92
BOSS Correlation Function analysis from the Effective Field Theory of Large-Scale Structure
Zhang, P., D’Amico, G., Senatore, L., Zhao, C., & Cai, Y.-F. (2022) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2022/02/036 · Cited by 92
A Step in understanding the Hubble tension
Aloni, D., Berlin, A., Joseph, M., Schmaltz, M., & Weiner, N. (2022) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.105.123516 · Cited by 91
Kirkby, D. P., Margala, D., Slosar, A., Bailey, S., Busca, N. G., Delubac, T., Rich, J., Bautista, J., Blomqvist, M., Brownstein, J. R., et al. (2013) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2013/03/024 · Cited by 91
Constraints on deviations from ΛCDM within Horndeski gravity
Bellini, E., Cuesta, A. J., Jimenez, R., & Verde, L. (2016) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2016/02/053 · Cited by 91
“BAO have their origin in the sound waves of the baryon-photon plasma in the early Universe, which were later imprinted in the distribution of galaxies, which we have observed with galaxy surveys such as 6dFGS [70], BOSS [71, 72], or WiggleZ [5].”
MethodReconstructing gravity on cosmological scales
Raveri, M. (2020) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.101.083524 · Cited by 91
Dynamical dark energy after Planck CMB final release and H 0 tension
Yang, W., Valentino, E. D., Pan, S., Wu, Y., & Lu, J. (2020) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/staa3914 · Cited by 87
Testing Screened Modified Gravity
Brax, P., Casas, S., Desmond, H., & Elder, B. (2021) · Universe · doi:10.3390/universe8010011 · Cited by 113
Galactic rotation curves in hybrid metric-Palatini gravity
Capozzıello, S., Harko, T., Koivisto, T., Lobo, F. S. N., & Olmo, G. J. (2013) · Astroparticle Physics · doi:10.1016/j.astropartphys.2013.09.005 · Cited by 90
Standard Rulers, Candles, and Clocks from the Low-Redshift Universe
Heavens, A., Jiménez, R., & Verde, L. (2014) · Physical Review Letters · doi:10.1103/physrevlett.113.241302 · Cited by 90
The length of the low-redshift standard ruler
Verde, L., Bernal, J. L., Heavens, A., & Jiménez, R. (2017) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stx116 · Cited by 90
“Constraints on the BAO are from the following galaxy surveys: Six Degree Field Galaxy Survey (Beutler et al. 2011), the LOWZ and CMASS galaxy samples of the Baryon Oscillation Spectroscopic Survey (BOSS-LOWZ and BOSS-CMASS, respectively; Cuesta et al. 2016, we use the isotropic measurement) and the…”
MethodGerbino, M., Katherine Freese, B., Vagnozzi, S., Lattanzi, M., Mena, O., Giusarma, E., & Ho, S. (2017) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.95.043512 · Cited by 90
Angular Baryon Acoustic Oscillation measure at z =2.225 from the SDSS quasar survey
de Carvalho, E., Bernui, A., Carvalho, G. C., Novaes, C. P., & Xavier, H. S. (2018) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2018/04/064 · Cited by 90
Domínguez, A., Wojtak, R., Finke, J., Ajello, M., Helgason, K., Prada, F., Desai, A., Paliya, V., Marcotulli, L., & Hartmann, D. H. (2019) · The Astrophysical Journal · doi:10.3847/1538-4357/ab4a0e · Cited by 90
“…2015) measured at redshifts z=0.38, 0.5, and 0.61 using prereconstruction (independent of cosmological model) methods (Alam et al. 2017), distance measurements from the 6dF survey at z=0.106 (Beutler et al. 2011) and from the Main Galaxy Sample of the SDSS (SDSS-MGS) at z=0.15 (Ross et al. 2015).”
MethodInfluentialA divergence-free parametrization of deceleration parameter for scalar field dark energy
Mamon, A. A., & Das, S. (2016) · International Journal of Modern Physics D · doi:10.1142/s0218271816500322 · Cited by 96
Om diagnostic applied to scalar field models and slowing down of cosmic acceleration
Shahalam, M., Sami, S., & Agarwal, A. (2015) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stv083 · Cited by 89
“(41) Next, we use BAO data of dA(z⋆) DV (ZBAO) (Eisenstein et al. 2005; Percival et al. 2010; Beutler et al. 2011; Blake et al. 2011; Jarosik et al. 2011; Giostri et al. 2012), where z⋆ ≈ 1091 is the decoupling time, dA(z) = ∫ z 0 dz′ H(z′) is the co-moving angular-diameter distance and DV (z) =…”
BackgroundMethodFrom Planck Data to Planck Era: Observational Tests of Holographic Cosmology
Afshordi, N., Claudio Corianò, A., Rose, L. D., Gould, E., & Skenderis, K. (2017) · Physical Review Letters · doi:10.1103/physrevlett.118.041301 · Cited by 91
Poulin, V., Bernal, J. L., Kovetz, E. D., & Kamionkowski, M. (2023) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.107.123538 · Cited by 89
“106 [75] and Ly-α auto-correalation and cross-correlation with QSO at z = 2 .”
BackgroundHUBBLE PARAMETER MEASUREMENT CONSTRAINTS ON DARK ENERGY
Farooq, O., Mania, D., & Ratra, B. (2013) · The Astrophysical Journal · doi:10.1088/0004-637x/764/2/138 · Cited by 88
“We also use the 6dFGS and SDSS data, three measurements from Beutler et al. (2011) and Percival et al. (2010), listed in Blake et al. (2011).”
BackgroundMethodDark sectors with dynamical coupling
Yang, W., Mena, O., Pan, S., & Valentino, E. D. (2019) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.100.083509 · Cited by 82
“[67, 68, 69].”
White, M. J., Zhou, R., DeRose, J., Ferraro, S., Chen, S.-F., Kokron, N., Bailey, S., Brooks, D., García-Bellido, J., Guy, J., et al. (2022) · UCL Discovery (University College London) · Cited by 88
Dark Sky Simulations: Early Data ReleasePreprint
Skillman, S. W., Warren, M. S., Turk, M., Wechsler, R. H., HOLZ, D. E., & Sutter, P. M. (2014) · arXiv (Cornell University) · doi:10.48550/arxiv.1407.2600 · Cited by 88
“We also use a better-constrained input cosmology (Beutler et al. 2011; Bennett et al. 2012; Anderson et al. 2014; Delubac et al. 2014; BICEP2Collaboration et al. 2014; Audren et al. 2012; Warren 2014), reducing the effects of non-universality in applying the Tinker et al. (2008) mass function to the…”
BackgroundMethodZhao, G., Saito, S., Percival, W. J., Ross, A. J., Montesano, F., Viel, M., Schneider, D. P., Manera, M., Miralda‐Escudé, J., Palanque‐Delabrouille, N., et al. (2013) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stt1710 · Cited by 87
“We also combine the baryonic acoustic oscillations (BAO) measurements from 6dF (Beutler et al. 2011), SDSS-II (Percivalet l. 2010) and the WiggleZ survey (Blake et al. 2011).”
MethodBaryon acoustic oscillations from the SDSS DR10 galaxies angular correlation function
Carvalho, G. C., Bernui, A., Benetti, M., Carvalho, J., & Alcaniz, J. S. (2016) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.93.023530 · Cited by 87
The Taipan Galaxy Survey: Scientific Goals and Observing Strategy
da Cunha, E., Hopkins, A. M., Colless, M., Taylor, E. N., Blake, C., Howlett, C., Magoulas, C., Lucey, J. R., Lagos, C. D. P., Kuehn, K., et al. (2017) · Publications of the Astronomical Society of Australia · doi:10.1017/pasa.2017.41 · Cited by 87
“…motions in the local Universe (e.g. Springob et al. 2014; Scrimgeour et al. 2016), constraining cosmological models with increasing precision (e.g. Beutler et al. 2011; Blake et al. 2011b; Anderson et al. 2012; Johnson et al. 2014; Alam et al. 2016), and obtaining a census of the properties of…”
BackgroundMethodSelf-citationThe void size function in dynamical dark energy cosmologies
Verza, G., Pisani, A., Carbone, C., Hamaus, N., & Guzzo, L. (2019) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2019/12/040 · Cited by 87
Evidence for Suppression of Structure Growth in the Concordance Cosmological Model
Nguyen, N.-M., Dragan Huterer, A., & Wen, Y. (2023) · Physical Review Letters · doi:10.1103/physrevlett.131.111001 · Cited by 86
THE WEAK LENSING SIGNAL AND THE CLUSTERING OF BOSS GALAXIES. I. MEASUREMENTS
Miyatake, H., More, S., Mandelbaum, R., Takada, M., Spergel, D. N., Kneib, J., Schneider, D. P., Brinkmann, J., & Brownstein, J. R. (2015) · The Astrophysical Journal · doi:10.1088/0004-637x/806/1/1 · Cited by 86
“…) of the energy density of the universe; this conclusion is supported by a growing body of diverse observational astrophysical evidence (see e.g., Beutler et al. 2011; Blake et al. 2011; Sullivan et al. 2011; Anderson et al. 2012; Reid et al. 2012; Suzuki et al. 2012; Hinshaw et al. 2013;…”
Result
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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