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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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“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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MethodThe Design and Implementation of FFTW3
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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
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Items 701–800 of 1,006
Future constraints on dynamical dark-energy using gravitational-wave standard sirens
Du, M., Yang, W., Xu, L., Pan, S., & Mota, D. F. (2019) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.100.043535 · Cited by 54
“106 [51], (ii) the Main Galaxy Sample of Data Release 7 of Sloan Digital Sky Survey (SDSS-MGS) at zeff = 0.”
BackgroundDesigning Horndeski and the effective fluid approach
Arjona, R., Cardona, W., & Nesseris, S. (2019) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.100.063526 · Cited by 57
Probing elastic interactions in the dark sector and the role of S 8
Jiménez, J. B., Bettoni, D., Figueruelo, D., Pannia, F. A. T., & Tsujikawa, S. (2021) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.104.103503 · Cited by 53
Higgs-dilaton cosmology: An inflation–dark-energy connection and forecasts for future galaxy surveys
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Constraints on active and sterile neutrinos in an interacting dark energy cosmology
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Novel cosmological bounds on thermally-produced axion-like particles
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“We use the most recent Planck 2018 data of CMB temperature and polarization anisotropies [47] together with BAO data from galaxy surveys, consisting of BOSS DR12 [64], 6dFGS [98] and SDSS-MGS [99].”
MethodField-level Neural Network Emulator for Cosmological N-body Simulations
Jamieson, D., Li, Y., de Oliveira, R. A., Villaescusa-Navarro, F., Ho, S., & Spergel, D. N. (2023) · The Astrophysical Journal · doi:10.3847/1538-4357/acdb6c · Cited by 53
Dark radiation and interacting scenarios
Diamanti, R., Giusarma, E., Mena, O., Archidiacono, M., & MELCHIORRI, A. (2013) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.87.063509 · Cited by 53
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“[30], the main galaxy sample (MGS) measurement from Ref.”
BackgroundGrandis, S., Rapetti, D., Saro, A., Mohr, J. J., & Dietrich, J. P. (2016) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stw2028 · Cited by 52
“…et al. 2015; Efstathiou 2014; Riess et al. 2016), supernovae type Ia (Conley et al. 2011; Betoule et al. 2013), baryon acoustic oscilla- tions (BAO; Beutler et al. 2011; Ross et al. 2015; Anderson et al. 2014; Delubac et al. 2015), cluster gas mass fraction (Allen et al. 2008; Mantz et al.…”
BackgroundMethodAdams, C., & Blake, C. (2017) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stx1529 · Cited by 53
“Our redshift sample for calculating the galaxy overdensity MNRAS 000, 1–20 (2017) comes from the 6dFGS baryon acoustic oscillation analysis by Beutler et al. (2011), who selected galaxies with magnitude K ≤ 12.9 in regions of the sky that had a completeness value of 60% or greater, which yielded…”
MethodInfluentialSelf-citationEffective field description of the Anton-Schmidt cosmic fluid
Capozzıello, S., D’Agostino, R., Giambò, R., & Luongo, O. (2019) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.99.023532 · Cited by 57
LyaCoLoRe: synthetic datasets for current and future Lyman-α forest BAO surveys
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From a bounce to the dark energy era with F ( R ) gravity
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Arjona, R., & Nesseris, S. (2021) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.103.103539 · Cited by 52
“The different BAO data used in our analysis comes from 6dFGS [61], SDDS [57], BOSS CMASS [62], WiggleZ [56], MGS [63] and BOSS DR12 [64], DES [65], Lya [66], DR - 14 LRG [67] and quasars [68].”
MethodCONSTRAINTS ON HYBRID METRIC-PALATINI GRAVITY FROM BACKGROUND EVOLUTION
Lima, N. A., & Smer-Barreto, V. (2016) · The Astrophysical Journal · doi:10.3847/0004-637x/818/2/186 · Cited by 52
“…analysis (Ade et al. 2013), we have used BAO observations from the 6dF Galaxy Redshift Survey (6dFGRS) at low redshift, dobs(z=0.106)=0.336±0.015 (Beutler et al. 2011), from the Luminous Red Galaxies sample of the Sloan Digital Sky Survey 7-year data release at the median redshift, dobs…”
MethodInfluentialComparison between different methods of model selection in cosmology
Rezaei, M., & Malekjani, M. (2021) · The European Physical Journal Plus · doi:10.1140/epjp/s13360-021-01200-w · Cited by 56
White paper on light sterile neutrino searches and related phenomenology
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Exploring massive neutrinos in dark cosmologies with eftcamb/EFTCosmoMC
Hu, B., Raveri, M., Silvestri, A., & Frusciante, N. (2015) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.91.063524 · Cited by 52
Constraining supersymmetry using the relic density and the Higgs boson
Versillé, S., Lafaye, R., Plehn, T., Rauch, M., Zerwas, D., Plaszczynski, S., Rouillé-d'Orfeuil, B., & Spinelli, M. (2014) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.89.055017 · Cited by 52
Probing cosmology with weak lensing selected clusters – I. Halo approach and all-sky simulations
Shirasaki, M., Hamana, T., & Yoshida, N. (2015) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stv1854 · Cited by 43
“…of astronomical observations such as Type Ia supernovae (e.g., Betoule et al. 2014), measurement of baryon acoustic oscillations in galaxy surveys (e.g., Beutler et al. 2011; Blake et al. 2011; Anderson et al. 2014), anisotropies of the cosmic microwave background (CMB) (e.g., Hinshaw et al. ?”
BackgroundCosmology with nonminimal kinetic coupling and a power-law potential
Skugoreva, M. A., Sushkov, S. V., & TOPORENSKY, A. V. (2013) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.88.083539 · Cited by 61
Tutusaus, I., Lamine, B., & Blanchard, A. (2019) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201833032 · Cited by 52
On structure formation from a small-scales-interacting dark sector
Asghari, M., Jiménez, J. B., Khosravi, S., & Mota, D. F. (2019) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2019/04/042 · Cited by 52
“In this analysis we use six likelihoods: the Planck likelihood containing high-`, low-` and lensing data provided with the Planck Legacy Archive2 [5], the Planck-SZ likelihood for the Sunyaev-Zeldovich effect measured by Planck [98, 99], the CFHTLenS likelihood with the weak lensing data [100, 101], the JLA likelihood…”
MethodForecasting interacting vacuum-energy models using gravitational waves
Yang, W., Pan, S., Valentino, E. D., Wang, B., & Wang, A. (2020) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2020/05/050 · Cited by 52
“[85] F.”
MethodTesting the equation of state for viscous dark energy
Odintsov, S. D., Gómez, D. S.-C., & Sharov, G. S. (2020) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.101.044010 · Cited by 52
Abdullah, M. H., Klypin, A. A., & Wilson, G. (2020) · The Astrophysical Journal · doi:10.3847/1538-4357/aba619 · Cited by 52
“We also use angular diameter distances as probed by Baryon Acoustic Oscillations (BAO) including the 6dF Galaxy Survey (Beutler et al. 2011), the SDSS Data Release 7 (Ross et al. 2015), and the BOSS Data Release 12 (Alam et al. 2017).”
MethodAccelerating universe in hybrid and logarithmic teleparallel gravity
Mandal, S., Bhattacharjee, S., Pacif, S. K. J., & Sahoo, P. K. (2020) · Physics of the Dark Universe · doi:10.1016/j.dark.2020.100551 · Cited by 55
Kinematic constraints beyond z ≃ 0 using calibrated GRB correlations
Luongo, O., & Muccino, M. (2020) · Astronomy and Astrophysics · doi:10.1051/0004-6361/202038264 · Cited by 55
Modeling and testing the equation of state for (Early) dark energy
Nojiri, S., Odintsov, S. D., Gómez, D. S.-C., & Sharov, G. S. (2021) · Physics of the Dark Universe · doi:10.1016/j.dark.2021.100837 · Cited by 52
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“…2011) Baryonic Oscillation Spectroscopic Survey (BOSS; Dawson et al. 2013), have reported detections of the baryonic acoustic feature at z > 0.5 (Blake et al. 2011b,d; Anderson et al. 2012; Sánchez et al. 2012), as well as the 6dF Galaxy Survey (Jones et al. 2009) at z < 0.2 (Beutler et al. 2011).”
BackgroundInfluentialSelf-citationImproved Hot Dark Matter Bound on the QCD Axion
Notari, A., Rompineve, F., & Giovanni Villadoro, A. (2023) · Physical Review Letters · doi:10.1103/physrevlett.131.011004 · Cited by 51
“106 [78], from the MGS galaxy sample of SDSS at z = 0.”
BackgroundProbing the neutrino mass hierarchy with cosmic microwave background weak lensing
Hall, A. C., & Challinor, A. D. (2012) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2012.21493.x · Cited by 51
“Current measurements of BAO are limited to the spherically-averaged correlation function (or power spectrum) which is sensitive to an effectiv distance[d2A(z)/H(z)] 1/3; see, for example, Beutler et al. (2011); Blake et al. (2011); Anderson et al. (2012) for the most recent measurements.”
BackgroundHořava Gravity in the Effective Field Theory formalism: From cosmology to observational constraints
Frusciante, N., Raveri, M., Vernieri, D., Hu, B., & Silvestri, A. (2016) · Physics of the Dark Universe · doi:10.1016/j.dark.2016.03.002 · Cited by 57
“106 [83].”
Testing Hu–Sawickif(R) gravity with the effective field theory approach
Hu, B., Raveri, M., Rizzato, M., & Silvestri, A. (2016) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stw775 · Cited by 51
“…oscillations (BAO) measurements taken from the SDSS Main Galaxy Sample at zeff = 0.15 (Ross et al. 2015), the BOSS DR11 ‘LOWZ’ sample at zeff = 0.32 (Anderson et al. 2014), the BOSS DR11 CMASS at zeff = 0.57 of Anderson et al. (2014) and the 6dFGS survey at zeff = 0.106 (Beutler et al. 2011).”
MethodInfluentialCONSTRAINING THE PROPERTIES OF DARK MATTER WITH OBSERVATIONS OF THE COSMIC MICROWAVE BACKGROUND
Thomas, D. B., Kopp, M., & Skordis, C. (2016) · The Astrophysical Journal · doi:10.3847/0004-637x/830/2/155 · Cited by 51
“2011) and Baryon Acoustic Oscillation (BAO) data (Anderson et al. 2014; Beutler et al. 2011).”
BackgroundMethodSpeeding upN-body simulations of modified gravity: chameleon screening models
Bose, S., Li, B., Barreira, A., He, J.-H., Hellwing, W. A., Koyama, K., Llinares, C., & Zhao, G. (2017) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2017/02/050 · Cited by 51
Search for sterile neutrinos in a universe of vacuum energy interacting with cold dark matter
Feng, L., Zhang, J.-F., & Zhang, X. (2019) · Physics of the Dark Universe · doi:10.1016/j.dark.2018.100261 · Cited by 51
Cosmological constraints of phantom dark energy models
Bouali, A., Albarran, I., Bouhmadi-López, M., & Ouali, T. (2019) · Physics of the Dark Universe · doi:10.1016/j.dark.2019.100391 · Cited by 51
Gaussian processes reconstruction of modified gravitational wave propagation
Belgacem, E., Foffa, S., Maggiore, M., & Yang, T. (2020) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.101.063505 · Cited by 51
Cosmological constraints on multi-interacting dark matter
Becker, N., Hooper, D. C., Kahlhöfer, F. K. D., Julien Lesgourgues, A., & Schöneberg, N. (2021) · RWTH Publications (RWTH Aachen) · Cited by 51
Hints, neutrino bounds, and WDM constraints from SDSS DR14 Lyman-α and Planck full-survey data
Palanque‐Delabrouille, N., Yèche, C., Schöneberg, N., Julien Lesgourgues, A., Walther, M., Chabanier, S., & Armengaud, E. (2020) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2020/04/038 · Cited by 263
Gerbino, M., Lattanzi, M., Mena, O., & Katherine Freese, B. (2017) · Physics Letters B · doi:10.1016/j.physletb.2017.10.052 · Cited by 50
Constraints on interacting dark energy models from time-delay cosmography with seven lensed quasars
Wang, L.-F., Zhang, J.-H., He, D.-Z., Zhang, J., & Zhang, X. (2022) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stac1468 · Cited by 52
Zhang, J., Geng, J.-J., & Zhang, X. (2014) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2014/10/044 · Cited by 50
“1) [42], SDSS-DR7 (z = 0.”
Johnson, A., Blake, C., Dossett, J. N., Koda, J., Parkinson, D., & Joudaki, S. (2016) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stw447 · Cited by 51
“To constrain the expansion history we use the following BAO measurements: WiggleZ reconstructed from Kazin et al. (2014), reconstructed DR11–CMASS and DR11–LOWZ from Anderson et al. (2014b), and the 6dFGS measurement from Beutler et al. (2011).”
MethodSelf-citationPlanck data versus large scale structure: Methods to quantify discordance
Charnock, T., Battye, R. A., & Moss, A. (2017) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.95.123535 · Cited by 50
Wang, L.-F., Zhao, Z.-W., Zhang, J., & Zhang, X. (2020) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2020/11/012 · Cited by 50
“106 [69], the SDSS main galaxy sample (MGS) at zeff = 0.”
BackgroundThe full Boltzmann hierarchy for dark matter-massive neutrino interactions
Mosbech, M. R., Bœhm, C., Hannestad, S., Mena, O., Stadler, J., & Wong, Y. Y. Y. (2021) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2021/03/066 · Cited by 50
“Most notably, there is a disagreement at more than 4σ [16, 17] between the value of H0 determined from early [18–23] and late-type [24–27] cosmological probes, with the latter favouring higher values.”
BackgroundEarly dark energy in the pre- and postrecombination epochs
Gómez-Valent, A., Zheng, Z., Amendola, L., Pettorino, V., & WETTERICH, C. (2021) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.104.083536 · Cited by 51
Quasidilaton nonlinear massive gravity: Investigations of background cosmological dynamics
Gannouji, R., Hossain, M. W., Sami, M., & Saridakis, E. N. (2013) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.87.123536 · Cited by 49
Observational Constraints on Dynamical Dark Energy with Pivoting Redshift
Yang, W., Pan, S., Valentino, E. D., & Saridakis, E. N. (2019) · Universe · doi:10.3390/universe5110219 · Cited by 49
“106 [61], the Main Galaxy Sample of Data Release 7 of Sloan Digital Sky Survey (SDSS-MGS) at zeff = 0.”
BackgroundAccelerating expansion of the universe in modified symmetric teleparallel gravity
Solanki, R., De, A., Mandal, S., & Sahoo, P. K. (2022) · Physics of the Dark Universe · doi:10.1016/j.dark.2022.101053 · Cited by 49
Katherine Freese, B., & Winkler, M. W. (2021) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.104.083533 · Cited by 49
The role of LRG1 and LRG2’s monopole in inferring the DESI 2024 BAO cosmology
Wang, Z., Lin, S., Ding, Z., & Hu, B. (2024) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stae2309 · Cited by 49
Phantom dark energy as an effect of bulk viscosity
Velten, H. E. S., Wang, J., & Meng, X.-H. (2013) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.88.123504 · Cited by 49
Neveu, J., Ruhlmann-Kleider, V., Conley, A., Palanque‐Delabrouille, N., Astier, P., Guy, J., & Babichev, E. (2013) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201321256 · Cited by 49
Cao, S., & Liang, N. (2013) · International Journal of Modern Physics D · doi:10.1142/s021827181350082x · Cited by 49
Versillé, S., Robinet, F., Leroy, N., Plaszczynski, S., Arnaud, N., Bizouard, M. A., Cavalier, F., Christensen, N. L., Couchot, F., Franco, S., et al. (2015) · Classical and Quantum Gravity · doi:10.1088/0264-9381/32/4/045003 · Cited by 49
Veropalumbo, A., Marulli, F., Moscardini, L., Moresco, M., & Cimatti, A. (2014) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stu1050 · Cited by 49
“…samples of galaxies (e.g. Eisenstein et al. 2005; Cole et al. 2005; Percival et al. 2007, 2010; Sánchez et al. 2009; Kazin et al. 2010; Beutler et al. 2011; Blake et al. 2011; Padmanabhan et al. 2012; Anderson et al. 2012, 2014) at low redshifts, z < 1, and with Lyα forest in quasar…”
BackgroundMethodBayesian 3D velocity field reconstruction with virbius
Lavaux, G. (2016) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stv2915 · Cited by 49
“This era will continue with TAIPAN (Beutler et al. 2011) and WALLABY (Duffy et al. 2012).”
MethodDetecting the neutrinos mass hierarchy from cosmological data
Xu, L., & Huang, Q.-G. (2017) · Science China Physics Mechanics and Astronomy · doi:10.1007/s11433-017-9125-0 · Cited by 49
Cosmological constraints with self-interacting sterile neutrinos
Song, N., González-García, M. C., & Salvadó, J. (2018) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2018/10/055 · Cited by 49
“We also include the measurements of the scale of the baryon acoustic oscillation (BAO) peaks at different red shifts as measured in the 6dF Galaxy Survey [73], the SDSS DR7 main Galaxy samples [74], the CMASS [75] and LOWZ [76] samples from SDSS DR11 results of BOSS experiment.”
MethodScreened fifth forces lower the TRGB-calibrated Hubble constant too
Desmond, H., & Sakstein, J. (2020) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.102.023007 · Cited by 49
Standard-siren Cosmology Using Gravitational Waves from Binary Black Holes
You, Z.-Q., Zhu, X. J., Ashton, G., Thrane, E., & Zhu, Z. (2021) · The Astrophysical Journal · doi:10.3847/1538-4357/abd4d4 · Cited by 49
Emergent Dark Energy, neutrinos and cosmological tensions
Yang, W., Valentino, E. D., Pan, S., & Mena, O. (2020) · Physics of the Dark Universe · doi:10.1016/j.dark.2020.100762 · Cited by 49
Cosmological constraints on slow roll inflation: An update
Forconi, M., Giarè, W., Di Valentino, E., & Melchiorri, A. (2021) · Physical Review D · doi:10.1103/physrevd.104.103528 · Cited by 48
Lorenz, C. S., Funcke, L., Calabrese, E., & Hannestad, S. (2019) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.99.023501 · Cited by 55
Simple-graduated dark energy and spatial curvature
Acquaviva, G., Akarsu, Ö., Katırcı, N., & Vazquez, J. A. (2021) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.104.023505 · Cited by 48
Mirror twin Higgs cosmology: constraints and a possible resolution to the H0 and S8 tensions
Bansal, S., Kim, J. H., Kolda, C., Low, M., & Tsai, Y. (2022) · Journal of High Energy Physics · doi:10.1007/jhep05(2022)050 · Cited by 47
Valentino, E. D., Giarè, W., MELCHIORRI, A., & Silk, J. I. (2022) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.106.103506 · Cited by 46
Dynamical dark energy in the light of DESI 2024 data
Roy, N. (2025) · Physics of the Dark Universe · doi:10.1016/j.dark.2025.101912 · Cited by 48
“The early universe measurements like CMB from Planck collaboration [4], BAO [7, 16, 1, 40], and BBN [8] data estimated the current value of the Hubble constant to be H 0 ∼ (67 .”
Neutrino Physics from the Cosmic Microwave Background and Large-Scale Structure
Abazajian, K. N., & Kaplinghat, M. (2016) · Annual Review of Nuclear and Particle Science · doi:10.1146/annurev-nucl-102014-021908 · Cited by 48
REDSHIFT MEASUREMENT AND SPECTRAL CLASSIFICATION FOR eBOSS GALAXIES WITH THE REDMONSTER SOFTWARE
Hutchinson, T. A., Bolton, A. S., Dawson, K. S., Prieto, C. A., Bailey, S., Bautista, J., Brownstein, J. R., Conroy, C., Guy, J., Myers, A. D., et al. (2016) · The Astronomical Journal · doi:10.3847/0004-6256/152/6/205 · Cited by 48
“…cosmic microwave background, redshift surveys can also be used to place constraints on cosmological parameters, such as the Hubble constant ( e.g., Beutler et al. 2011 ) and the dark energy equation of state through measurements of the baryon acoustic oscillation ( BAO ) peak, fi rst detected in…”
Li, X.-D., Park, C., Sabiu, C. G., Park, H., Weinberg, D. H., Schneider, D. P., Kim, J., & Hong, S. E. (2016) · The Astrophysical Journal · doi:10.3847/0004-637x/832/2/103 · Cited by 48
“…uses the BAO feature in the clustering of galaxies on scales of 100-150 datasets include three sets of measurements from SDSS DR11 (Anderson et al. 2013), 6dFGS (Beutler et al. 2011) and SDSS MGS (Ross et al. 2015) h−1Mpc created by the oscillation of the baryon-photon plasma in the early Universe.”
MethodCosmological aspects of a hyperbolic solution in f(R,T) gravity
Nagpal, R., Singh, J. K., Beesham, A., & Shabani, H. (2019) · Annals of Physics · doi:10.1016/j.aop.2019.03.015 · Cited by 48
Forecast for FAST: from galaxies survey to intensity mapping
Hu, W., Wang, X., Wu, F., Wang, Y., Zhang, P., & Chen, X. (2020) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/staa650 · Cited by 48
“…acoustic oscillation (BAO) features in the galaxy power spectrum are measured, and used as standard rulers to constrain cosmological models (Eisenstein et al. 2005; Cole et al. 2005; Percival et al. 2010; Beutler et al. 2011; Blake et al. 2011; Ross et al. 2015; Alam et al. 2017; Ata et al. 2018).”
MethodGravity in the infrared and effective nonlocal models
Belgacem, E., Dirian, Y., Finke, A., Foffa, S., & Maggiore, M. (2020) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2020/04/010 · Cited by 55
“• For BAO we still use the likelihoods of the BAO detection of the 6dF Galaxy Survey [128] and the BAO scale measurement of SDSS DR7 Main Galaxy Sample [129], and we update the SDSS data using the power spectrum of BAO from the Data Release 12 [130].”
MethodA Bayesian comparison between $$\Lambda $$CDM and phenomenologically emergent dark energy models
Rezaei, M., Naderi, T., Malekjani, M., & Mehrabi, A. (2020) · The European Physical Journal C · doi:10.1140/epjc/s10052-020-7942-6 · Cited by 48
Agrawal, P., Cyr-Racine, F.-Y., Randall, L., & Scholtz, J. (2017) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2017/08/021 · Cited by 48
New cosmological bounds on hot relics: axions and neutrinos
Giarè, W., Valentino, E. D., MELCHIORRI, A., & Mena, O. (2021) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stab1442 · Cited by 47
Zhao, M.-M., Li, Y., Zhang, J., & Zhang, X. (2017) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stx978 · Cited by 47
“We use the BAOs data in good agreement with the Planck data, including the measurements from the 6dFGS (zeff = 0.1) (Beutler et al. 2011), SDSS-MGS (zeff = 0.15) (Ross et al. 2015), LOWZ (zeff = 0.32) and CMASS (zeff = 0.57) samples of BOSS (Anderson et al. 2014).”
MethodInfluentialOne likelihood to bind them all: Lyman-α constraints on non-standard dark matter
Hooper, D. C., Schöneberg, N., Murgia, R., Archidiacono, M., Julien Lesgourgues, A., & Viel, M. (2022) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2022/10/032 · Cited by 47
Early dark energy with power-law F(R) gravity
Odintsov, S. D., Oikonomou, V. K., & Sharov, G. S. (2023) · Physics Letters B · doi:10.1016/j.physletb.2023.137988 · Cited by 47
Cosmology with matter diffusion
Calogero, S., & Velten, H. E. S. (2013) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2013/11/025 · Cited by 49
Massive photon and dark energy
Kouwn, S., Oh, P., & Park, C. (2016) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.93.083012 · Cited by 48
“(4.72) As the BAO parameter, we use six numbers of rs(zd)/DV (z) extracted from the SixDegree-Field Galaxy Survey [32], the Sloan Digital Sky Survey Data Release 7 and 9 [33], and the WiggleZ Dark Energy Survey [34], where rs(z) is the comoving sound horizon size.”
MethodInfluentialA Measurement of the Hubble Constant Using Galaxy Redshift Surveys
Wang, Y., Xu, L., & Zhao, G.-B. (2017) · The Astrophysical Journal · doi:10.3847/1538-4357/aa8f48 · Cited by 47
Latest astronomical constraints on some non-linear parametric dark energy models
Yang, W., Pan, S., & Paliathanasis, A. (2018) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/sty019 · Cited by 47
A new test of f(R) gravity with the cosmological standard rulers in radio quasars
Xu, T., Cao, S., Qi, J., Biesiada, M., Zheng, X., & Zhu, Z. (2018) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2018/06/042 · Cited by 47
New parametrized equation of state for dark energy surveys
Jaime, L. G., Jaber, M., & Escamilla‐Rivera, C. (2018) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.98.083530 · Cited by 47
Efficient computation of galaxy bias with neutrinos and other relics
Muñoz, J. B., & Dvorkin, C. (2018) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.98.043503 · Cited by 47
Constraints on quintessence scalar field models using cosmological observations
Yang, W.-Q., Shahalam, M., Pal, B., Pan, S., & Wang, A.-Z. (2018) · Physical Review D · doi:10.1103/physrevd.100.023522 · Cited by 40
“However, in the present work we shall consider some specific potentials for quintessence scalar field models aiming to impose stringent cosmological constraints using the latest cosmological sources, namely, the cosmic microwave background temperature and polarization data [75, 76], baryon acoustic oscillations distan…”
BackgroundMethodDark energy survey year 1 results: Constraining baryonic physics in the Universe
Huang, H.-J., Eifler, T. F., Mandelbaum, R., Bernstein, G. M., Chen, A., Choi, A., García-Bellido, J., Dragan Huterer, A., Krause, E., Rozo, E., et al. (2021) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stab357 · Cited by 47
“(Beutler et al. 2011; Ross et al. 2015; Alam et al. 2017).”
MethodInfluentialHorava Gravity in the Effective Field Theory formalism: From cosmology to observational constraints
Frusciante, N., Raveri, M., Vernieri, D., Hu, B., & Silvestri, A. (2016) · Leiden Repository (Leiden University) · Cited by 47
Gonzalez, J. E., Benetti, M., von Marttens, R., & Alcaniz, J. S. (2021) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2021/11/060 · Cited by 47
“Following the analysis of the latest Planck release [2], we use the BAO measurements from 6dFGS [28], SDSS-MGS [29], and BOSS DR12 [30] surveys;”
MethodConstraints on prerecombination early dark energy from SPT-3G public data
Posta, A. L., Louis, T., Garrido, X., & Hill, J. C. (2022) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.105.083519 · Cited by 46
Abbott, T. M. C., Adamów, M., Aguena, M., Allam, S., Alves, O., Amon, A., Andrade-Oliveira, F., Asorey, J., Avila, S., Bacon, D., et al. (2024) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.110.063515 · Cited by 46
Priors on the effective dark energy equation of state in scalar-tensor theories
Raveri, M., Bull, P., Silvestri, A., & Pogosian, L. (2017) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.96.083509 · Cited by 46
Olivari, L. C., Dickinson, C., Battye, R. A., Ma, Y.-Z., Costa, A. A., Remazeilles, M., & Harper, S. (2017) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stx2621 · Cited by 46
“…showed that by using the Planck temperature, polarization and lensing data, the 6dFGS, SDSS-MGS, and BOSS-LOWZ BAO measurements of DV /rdrag (Beutler et al. 2011; Ross et al. 2015; Anderson et al. 2014), the CMASS-DR11 anisotropic BAO measurements of Anderson et al. (2014), the JLA…”
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
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