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.
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
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.
Cites
The Sloan Digital Sky Survey: Technical Summary
York, D. G., Adelman-McCarthy, J., Anderson, J. E., Anderson, S. F., Annis, J., Bahcall, N. A., Bakken, J. A., Barkhouser, R. H., Bastian, S., Berman, E., et al. (2000) · The Astronomical Journal · doi:10.1086/301513 · Cited by 10,392 · cited 1× · see citing works
“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.”
MethodKomatsu, 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 · see citing works
FIVE-YEAR<i>WILKINSON MICROWAVE ANISOTROPY PROBE</i>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 · see citing works
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× · see citing works
“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 · see citing works
Lewis, A., Challinor, A., & Lasenby, A. (2000) · The Astrophysical Journal · doi:10.1086/309179 · Cited by 4,920 · see citing works
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× · see citing works
“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 · see citing works
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× · see citing works
“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 · see citing works
The 2dF Galaxy Redshift Survey: spectra and redshifts
Colless, M., Dalton, G., Maddox, S., Sutherland, W. J., Norberg, P., Cole, S., Bland‐Hawthorn, J., Bridges, T. J., Cannon, R., Collins, C. A., et al. (2001) · Monthly Notices of the Royal Astronomical Society · doi:10.1046/j.1365-8711.2001.04902.x · Cited by 2,368 · cited 2× · see citing works
“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.”
MethodSelf-citationBaryonic Features in the Matter Transfer Function
Eisenstein, D. J., & Hu, W. (1998) · The Astrophysical Journal · doi:10.1086/305424 · Cited by 2,250 · cited 3× · see citing works
“During the fit we calculate rs(zd) using the fitting formula of Eisenstein & Hu (1998).”
BackgroundMethodInfluentialCole, S., Percival, W. J., Peacock, J. A., Norberg, P., Baugh, C. M., Frenk, C. S., Baldry, I. K., Bland‐Hawthorn, J., Bridges, T., Cannon, R., et al. (2005) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2005.09318.x · Cited by 2,100 · cited 2× · see citing works
“…function ξ(s) (Martinez 2009; Gaztanaga, Cabre & Hui 2009; Labini et al. 2009; Sanchez et al. 2009; Kazin et al. 2010), the power spectrum P (k) (Cole et al. 2005; Tegmark et al. 2006; Huetsi 2006; Reid et al. 2010), the projected correlation function w(rp) of photometric redshift samples…”
BackgroundMethodSelf-citationStable clustering, the halo model and non-linear cosmological power spectra
Smith, R. E., Peacock, J. A., Jenkins, A., White, S. D. M., Frenk, C. S., Pearce, F. R., Thomas, P. A., Efstathiou, G., & Couchman, H. M. P. (2003) · Monthly Notices of the Royal Astronomical Society · doi:10.1046/j.1365-8711.2003.06503.x · Cited by 2,054 · cited 1× · see citing works
“The nonlinear evolution of the power spectrum in CAMB is calculated using the halofit code (Smith et al. 2003).”
MethodBias and variance of angular correlation functions
Landy, S. D., & Szalay, A. S. (1993) · The Astrophysical Journal · doi:10.1086/172900 · Cited by 1,969 · cited 1× · see citing works
“The redshift correlation function itself is given by Landy & Szalay (1993): ξ′data(s) = 1 + DD(s) RR(s) ( nr nd )2 − 2DR(s) RR(s) ( nr nd ) , (4) where the ratio nr/nd is given by nr nd = ∑Nr i wi(~x) ∑Nd j wj(~x) (5) and the sums go over all random (Nr) and data (Nd) galaxies.”
MethodBaryon acoustic oscillations in the Sloan Digital Sky Survey Data Release 7 galaxy sample
Percival, W. J., Reid, B. A., Eisenstein, D. J., Bahcall, N. A., Budavari, T., Frieman, J. A., Fukugita, M., Gunn, J. E., Ivezić, Ž., Knapp, G. R., et al. (2010) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2009.15812.x · Cited by 1,846 · cited 6× · see citing works
“Subsequent studies using the final SDSS-LRG sample and combining it with the SDSS-main and the 2dFGRS sample were able to improve on this measurement and constrain the distance-redshift relation at zeff = 0.2 and zeff = 0.35 with 3% accuracy (Percival et al. 2010).”
MethodResultInfluentialRiess, A. G., Macri, L. M., Casertano, S., Lampeitl, H., Ferguson, H. C., Filippenko, A. V., Jha, S. W., Li, W., & Chornock, R. (2011) · The Astrophysical Journal · doi:10.1088/0004-637x/730/2/119 · Cited by 1,513 · cited 2× · see citing works
“The SH0ES program (Riess et al. 2011) determined the Hubble constant using the distance ladder method.”
MethodCosmological constraints from the SDSS luminous red galaxies
Tegmark, M., Eisenstein, D. J., Strauss, M. A., Weinberg, D. H., Blanton, M. R., Frieman, J. A., Fukugita, M., Gunn, J. E., Hamilton, A. J. S., Knapp, G. R., et al. (2006) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.74.123507 · Cited by 1,387 · cited 1× · see citing works
“…(Martinez 2009; Gaztanaga, Cabre & Hui 2009; Labini et al. 2009; Sanchez et al. 2009; Kazin et al. 2010), the power spectrum P (k) (Cole et al. 2005; Tegmark et al. 2006; Huetsi 2006; Reid et al. 2010), the projected correlation function w(rp) of photometric redshift samples (Padmanabhan et al.…”
BackgroundPrimeval Adiabatic Perturbation in an Expanding Universe
Peebles, P. J. E., & Yu, J. T. (1970) · The Astrophysical Journal · doi:10.1086/150713 · Cited by 1,230 · cited 1× · see citing works
“The radiation pressure drives sound-waves originating from overdensities in the matter distribution (Peebles & Yu 1970; ⋆ E-mail: florian.beutler@icrar.org Sunyaev & Zeldovich 1970; Bond & Efstathiou 1987).”
BackgroundA Cosmology Calculator for the World Wide Web
WRIGHT, E. L. (2006) · Publications of the Astronomical Society of the Pacific · doi:10.1086/510102 · Cited by 1,172 · cited 1× · see citing works
“Our fiducial model gives DfidV (zeff) = 440.5 Mpc, where we have followed the distance definitions of Wright (2006) throughout.”
BackgroundInfluentialSmall-scale fluctuations of relic radiation
Sunyaev, R. A., & Zel’dovich, Y. B. (1970) · Astrophysics and Space Science · doi:10.1007/bf00653471 · Cited by 1,114 · see citing works
The 6dF Galaxy Survey: final redshift release (DR3) and southern large-scale structures
Jones, D. H. P., Read, M., Saunders, W., Colless, M., Jarrett, T. H., Parker, Q. A., Fairall, A. P., Mauch, T., Sadler, E. M., Watson, F. G., et al. (2009) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2009.15338.x · Cited by 1,052 · cited 2× · see citing works
“Papers by Jones et al. (2004, 2006, 2009) describe 6dFGS in full detail, including comparisons between 6dFGS, 2dFGRS and SDSS. Galaxies were excluded from our sample if they resided in sky regions with completeness lower than 60 percent.”
MethodInfluentialSelf-citation2MASS Extended Source Catalog: Overview and Algorithms
Jarrett, T. H., Chester, T. J., Cutri, R. M., Schneider, S. E., Skrutskie, M. F., & Huchra, J. P. (2000) · The Astronomical Journal · doi:10.1086/301330 · Cited by 989 · cited 1× · see citing works
“The galaxies used in this analysis were selected to K 6 12.9 from the 2MASS Extended Source Catalog (2MASS XSC; Jarrett et al. 2000) and combined with redshift data from the 6dF Galaxy Survey (6dFGS; Jones et al. 2009).”
MethodInfluentialPower-spectrum analysis of three-dimensional redshift surveys
Feldman, H. A., Kaiser, N., & Peacock, J. A. (1994) · The Astrophysical Journal · doi:10.1086/174036 · Cited by 931 · see citing works
Probing Dark Energy with Baryonic Acoustic Oscillations from Future Large Galaxy Redshift Surveys
Seo, H., & Eisenstein, D. J. (2003) · The Astrophysical Journal · doi:10.1086/379122 · Cited by 797 · cited 1× · see citing works
“Very interesting for cosmology is the idea of using the sound horizon scale as a standard ruler (Eisenstein, Hu & Tegmark 1998; Cooray et al. 2001; Seo & Eisenstein 2003; Blake & Glazebrook 2003).”
BackgroundGAZTAÑAGA, E., Cabré, A., & Hui, L. (2009) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2009.15405.x · Cited by 635 · see citing works
The statistics of cosmic background radiation fluctuations
Bond, J. R., & Efstathiou, G. (1987) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/226.3.655 · Cited by 629 · cited 1× · see citing works
“The radiation pressure drives sound-waves originating from overdensities in the matter distribution (Peebles & Yu 1970; ⋆ E-mail: florian.beutler@icrar.org Sunyaev & Zeldovich 1970; Bond & Efstathiou 1987).”
BackgroundA lognormal model for the cosmological mass distribution
Coles, P., & Jones, B. J. T. (1991) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/248.1.1 · Cited by 605 · cited 1× · see citing works
“To obtain reliable error-bars for the correlation function we use log-normal realisations (Coles & Jones 1991; Cole et al. 2005; Kitaura et al. 2009).”
MethodThe 6dF Galaxy Survey: samples, observational techniques and the first data release
Jones, D. H., Saunders, W., Colless, M., Read, M. A., Parker, Q. A., Watson, F. G., Campbell, L., Burkey, D., Mauch, T., Moore, L., et al. (2004) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2004.08353.x · Cited by 561 · cited 1× · see citing works
“Papers by Jones et al. (2004, 2006, 2009) describe 6dFGS in full detail, including comparisons between 6dFGS, 2dFGRS and SDSS. Galaxies were excluded from our sample if they resided in sky regions with completeness lower than 60 percent.”
Self-citationPOWER SPECTRUM ANALYSIS OF THREE-DIMENSIONAL REDSHIFT SURVEYSPreprint
Feldman, H. A., Kaiser, N., & Peacock, J. A. (1993) · Cited by 537 · see citing works
Renormalized cosmological perturbation theory
Crocce, M., & Scoccimarro, R. (2006) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.73.063519 · Cited by 536 · cited 1× · see citing works
“c© 0000 RAS, MNRAS 000, 000–000 ory (Crocce & Scoccimarro 2006; Matsubara 2008) by k∗ = [ 1 6π2 ∫ ∞ 0 dk Plin(k) ]−1/2 , (19) where Plin(k) is again the linear power spectrum.”
Probing Dark Energy Using Baryonic Oscillations in the Galaxy Power Spectrum as a Cosmological Ruler
Blake, C., & Glazebrook, K. (2003) · The Astrophysical Journal · doi:10.1086/376983 · Cited by 535 · see citing works
Self-citationMatsubara, T. (2008) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.77.063530 · Cited by 491 · cited 1× · see citing works
“c© 0000 RAS, MNRAS 000, 000–000 ory (Crocce & Scoccimarro 2006; Matsubara 2008) by k∗ = [ 1 6π2 ∫ ∞ 0 dk Plin(k) ]−1/2 , (19) where Plin(k) is again the linear power spectrum.”
Reid, B., Percival, W. J., Eisenstein, D. J., Verde, L., Spergel, D. N., Skibba, R., Bahcall, N. A., Budavári, T., Frieman, J. A., Fukugita, M., et al. (2010) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2010.16276.x · Cited by 489 · cited 2× · see citing works
“…Hui 2009; Labini et al. 2009; Sanchez et al. 2009; Kazin et al. 2010), the power spectrum P (k) (Cole et al. 2005; Tegmark et al. 2006; Huetsi 2006; Reid et al. 2010), the projected correlation function w(rp) of photometric redshift samples (Padmanabhan et al. 2007; Blake et al. 2007) and a…”
BackgroundMethodInfluentialNonlinear evolution of baryon acoustic oscillations
Crocce, M., & Scoccimarro, R. (2008) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.77.023533 · Cited by 467 · cited 5× · see citing works
“Crocce & Scoccimarro (2008) used renormalised perturbation theory (RPT) and found percentlevel shifts in the BAO peak.”
BackgroundMethodInfluentialOn the Robustness of the Acoustic Scale in the Low‐Redshift Clustering of Matter
Eisenstein, D. J., Seo, H., & White, M. J. (2007) · The Astrophysical Journal · doi:10.1086/518755 · Cited by 460 · cited 1× · see citing works
“All non-linear effects influencing the correlation function can be approximated by a convolution with a Gaussian damping factor exp[−(rk∗/2)2] (Eisenstein et al. 2007; Eisenstein, Seo & White 2007), where k∗ is the damping scale.”
MethodImproving Cosmological Distance Measurements by Reconstruction of the Baryon Acoustic Peak
Eisenstein, D., Seo, H., Sirko, E., & Spergel, D. (2006) · The Astrophysical Journal · doi:10.1086/518712 · Cited by 456 · cited 1× · see citing works
“All non-linear effects influencing the correlation function can be approximated by a convolution with a Gaussian damping factor exp[−(rk∗/2)2] (Eisenstein et al. 2007; Eisenstein, Seo & White 2007), where k∗ is the damping scale.”
MethodEfstathiou, G., & Bond, J. R. (1999) · Monthly Notices of the Royal Astronomical Society · doi:10.1046/j.1365-8711.1999.02274.x · Cited by 402 · cited 1× · see citing works
“Measurements of other cosmological parameters often show degeneracies in the CMB data alone (Efstathiou & Bond 1999), especially in models with extra parameters beyond flat ΛCDM.”
BackgroundThick gas discs in faint dwarf galaxies
Roychowdhury, S., Chengalur, J. N., Begum, A., & Karachentsev, I. D. (2010) · Monthly Notices of the Royal Astronomical Society Letters · doi:10.1111/j.1745-3933.2010.00835.x · Cited by 394 · see citing works
The clustering of luminous red galaxies in the Sloan Digital Sky Survey imaging data
Padmanabhan, N., Schlegel, D. J., Seljak, U., Makarov, A., Bahcall, N. A., Blanton, M. R., Brinkmann, J. V., Eisenstein, D. J., Finkbeiner, D. P., Gunn, J. E., et al. (2007) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2007.11593.x · Cited by 360 · cited 1× · see citing works
“…et al. 2010), the power spectrum P (k) (Cole et al. 2005; Tegmark et al. 2006; Huetsi 2006; Reid et al. 2010), the projected correlation function w(rp) of photometric redshift samples (Padmanabhan et al. 2007; Blake et al. 2007) and a cluster sample based on the SDSS photometric data (Huetsi 2009).”
MethodMeasuring Cosmological Parameters with Galaxy Surveys
Tegmark, M. (1997) · Physical Review Letters · doi:10.1103/physrevlett.79.3806 · Cited by 353 · cited 2× · see citing works
“We calculated the effective volume of the survey using the estimate of Tegmark (1997) Veff = ∫ d3~x [ n(~x)P0 1 + n(~x)P0 ]2 (1) where n(~x) is the mean galaxy density at position ~x, determined from the data, and P0 is the characteristic power spectrum amplitude of the BAO signal.”
BackgroundMethodTHE COYOTE UNIVERSE. I. PRECISION DETERMINATION OF THE NONLINEAR MATTER POWER SPECTRUM
Heitmann, K., White, M. J., Wagner, C., Habib, S., & Higdon, D. (2010) · The Astrophysical Journal · doi:10.1088/0004-637x/715/1/104 · Cited by 321 · cited 1× · see citing works
“This code is calibrated by n-body simulations and can describe non-linear effects in the shape of the matter power spectrum for pure CDM models to an accuracy of around 5 − 10% (Heitmann et al. 2010).”
MethodNorberg, P., Baugh, C., Gaztañaga, E., & Croton, D. (2008) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2009.14389.x · Cited by 291 · see citing works
The Stromlo-APM redshift survey. 2: Variation of galaxy clustering with morphology and luminosity
Loveday, J., Maddox, S., Efstathiou, G., & Peterson, B. A. (1995) · The Astrophysical Journal · doi:10.1086/175453 · Cited by 275 · cited 1× · see citing works
“Other authors have used the so called J3-weighting which optimises the error over all scales by weighting each scale differently (e.g. Efstathiou 1988; Loveday et al. 1995).”
MethodImproving Cosmological Distance Measurements by Reconstruction of the Baryon Acoustic Peak
Eisenstein, D. J., Seo, H., Sirko, E., & Spergel, D. N. (2006) · CERN Document Server (European Organization for Nuclear Research) · Cited by 275 · see citing works
Efstathiou, G. P., & Bond, J. R. (1998) · CERN Document Server (European Organization for Nuclear Research) · Cited by 255 · see citing works
Eisenstein, D. J., Hu, W., & Tegmark, M. (1998) · The Astrophysical Journal · doi:10.1086/311582 · Cited by 252 · see citing works
Scale dependence of halo and galaxy bias: Effects in real space
Smith, R. C., Scoccimarro, R., & Sheth, R. K. (2007) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.75.063512 · Cited by 245 · cited 1× · see citing works
“However, several authors report possible shifts of up to 1% (Guzik & Bernstein 2007; Smith et al. 2008, 2007; Angulo et al. 2008).”
BackgroundKazin, E. A., Blanton, M. R., Scoccimarro, R., McBride, C. K., Berlind, A. A., Bahcall, N. A., Brinkmann, J., Czarapata, P. C., Frieman, J. A., Kent, S., et al. (2010) · The Astrophysical Journal · doi:10.1088/0004-637x/710/2/1444 · Cited by 234 · cited 3× · see citing works
“Another motivation for our study is that the SDSS data after data release 3 (DR3) show more correlation on large scales than expected by ΛCDM and have no sign of a crossover to negative ξ up to 200h−1 Mpc (the ΛCDM prediction is 140h−1 Mpc) (Kazin et al. 2010).”
BackgroundMethodResultThe Intermediate‐Scale Clustering of Luminous Red Galaxies
Zehavi, I., Eisenstein, D. J., Nichol, R. C., Blanton, M. R., Hogg, D. W., Brinkmann, J., Loveday, J., Meiksin, A. A., Schneider, D. P., & Tegmark, M. (2005) · The Astrophysical Journal · doi:10.1086/427495 · Cited by 209 · cited 1× · see citing works
“In a magnitude limited sample there is a correlation between luminosity and redshift, which establishes a correlation between bias and redshift (Zehavi et al. 2005).”
BackgroundThe detectability of baryonic acoustic oscillations in future galaxy surveys
Angulo, R. E., Baugh, C. M., Frenk, C. S., & Lacey, C. G. (2007) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2007.12587.x · Cited by 191 · see citing works
Blake, C., Collister, A., Bridle, S., & Lahav, O. (2007) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2006.11263.x · Cited by 162 · cited 1× · see citing works
“…et al. 2010), the power spectrum P (k) (Cole et al. 2005; Tegmark et al. 2006; Huetsi 2006; Reid et al. 2010), the projected correlation function w(rp) of photometric redshift samples (Padmanabhan et al. 2007; Blake et al. 2007) and a cluster sample based on the SDSS photometric data (Huetsi 2009).”
MethodSelf-citationCorrelation Function in Deep Redshift Space as a Cosmological Probe
Matsubara, T. (2004) · The Astrophysical Journal · doi:10.1086/424561 · Cited by 161 · cited 3× · see citing works
“The wide angle description of redshift space distortions has been laid out in several papers (Szalay et al. 1997; Szapudi 2004; Matsubara 2004; Papai & Szapudi 2008; Raccanelli et al. 2010), which we summarise in Appendix C.”
BackgroundBlake, C., Davis, T. M., Poole, G. B., Parkinson, D., Brough, S., Colless, M., Contreras, C., Couch, W. J., Croom, S. M., Drinkwater, M. J., et al. (2024) · doi:10.25916/sut.26215247.v1 · Cited by 155 · see citing works
Self-citationMotion of the acoustic peak in the correlation function
Smith, R. C., Scoccimarro, R., & Sheth, R. K. (2008) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.77.043525 · Cited by 152 · cited 1× · see citing works
“However, several authors report possible shifts of up to 1% (Guzik & Bernstein 2007; Smith et al. 2008, 2007; Angulo et al. 2008).”
BackgroundNear-infrared and optical luminosity functions from the 6dF Galaxy Survey
Jones, D. H. P., Peterson, B. A., Colless, M., & Saunders, W. (2006) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2006.10291.x · Cited by 150 · cited 2× · see citing works
“Papers by Jones et al. (2004, 2006, 2009) describe 6dFGS in full detail, including comparisons between 6dFGS, 2dFGRS and SDSS. Galaxies were excluded from our sample if they resided in sky regions with completeness lower than 60 percent.”
MethodSelf-citationChuang, C.-H., & Wang, Y. (2012) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2012.21565.x · Cited by 140 · cited 1× · see citing works
“While there are studies that report a successful (but very low signal-to-noise) detection in the 2D correlation function using the SDSS-LRG data (e.g. Gaztanaga, Cabre & Hui 2009; Chuang & Wang 2011, but see also Kazin et al. 2010), our sample does not allow this kind of analysis.”
MethodThe detectability of baryonic acoustic oscillations in future galaxy surveys
Angulo, R. E., Baugh, C. M., Frenk, C. S., & Lacey, C. G. (2007) · CERN Document Server (European Organization for Nuclear Research) · Cited by 138 · see citing works
Constraining anisotropic baryon oscillations
Padmanabhan, N., & White, M. J. (2008) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.77.123540 · Cited by 122 · cited 2× · see citing works
“It is defined as (Eisenstein et al. 2005; Padmanabhan & White 2008) α = DV (zeff) DfidV (zeff) .”
BackgroundMethodSánchez, A. G., Crocce, M., Cabre, A., Baugh, C. M., & GAZTAÑAGA, E. (2009) · Max Planck Digital Library · Cited by 113 · see citing works
Correlation Function in Deep Redshift Space as a Cosmological Probe
Matsubara, T. (2004) · CERN Document Server (European Organization for Nuclear Research) · Cited by 105 · see citing works
Fourier analysis of luminosity-dependent galaxy clustering
Percival, W. J., Verde, L., & Peacock, J. A. (2003) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2004.07245.x · Cited by 93 · see citing works
Non-perturbative effects of geometry in wide-angle redshift distortions
Pápai, P., & Szapudi, I. (2008) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2008.13572.x · Cited by 93 · cited 1× · see citing works
“The wide angle description of redshift space distortions has been laid out in several papers (Szalay et al. 1997; Szapudi 2004; Matsubara 2004; Papai & Szapudi 2008; Raccanelli et al. 2010), which we summarise in Appendix C.”
BackgroundWide‐Angle Redshift Distortions Revisited
Szapudi, I. (2004) · The Astrophysical Journal · doi:10.1086/423168 · Cited by 93 · cited 1× · see citing works
“The wide angle description of redshift space distortions has been laid out in several papers (Szalay et al. 1997; Szapudi 2004; Matsubara 2004; Papai & Szapudi 2008; Raccanelli et al. 2010), which we summarise in Appendix C.”
BackgroundWhat is the best way to measure baryonic acoustic oscillations?
Sánchez, A. G., Baugh, C. M., & Angulo, R. E. (2008) · Max Planck Digital Library · Cited by 93 · see citing works
Non-Gaussian fluctuations and the statistics of galaxy clustering
Weinberg, D. H., & Cole, S. (1992) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/259.4.652 · Cited by 88 · see citing works
Theoretical uncertainty in baryon oscillations
Eisenstein, D. J., & White, M. J. (2004) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.70.103523 · Cited by 78 · cited 1× · see citing works
“Beside the fact that the Hubble constant H0 cancels out in the determination of R, this ratio is also more robust against effects caused by possible extra relativistic species (Eisenstein & White 2004).”
BackgroundMeasuring Angular Diameter Distances through Halo Clustering
Cooray, A. R., Hu, W., Dragan Huterer, A., & Joffre, M. (2001) · The Astrophysical Journal · doi:10.1086/323323 · Cited by 74 · cited 1× · see citing works
“Very interesting for cosmology is the idea of using the sound horizon scale as a standard ruler (Eisenstein, Hu & Tegmark 1998; Cooray et al. 2001; Seo & Eisenstein 2003; Blake & Glazebrook 2003).”
BackgroundRecovering the non-linear density field from the galaxy distribution with a Poisson-lognormal filter
Kitaura, F.-S., Jasche, J., & Metcalf, R. B. (2010) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2009.16163.x · Cited by 73 · cited 1× · see citing works
“To obtain reliable error-bars for the correlation function we use log-normal realisations (Coles & Jones 1991; Cole et al. 2005; Kitaura et al. 2009).”
MethodFourier analysis of luminosity-dependent galaxy clusteringPreprint
Percival, W. J., Verde, L., & Peacock, J. A. (2003) · Cited by 67 · see citing works
Power spectrum of the maxBCG sample: detection of acoustic oscillations using galaxy clusters
Hütsi, G. (2009) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2009.15824.x · Cited by 65 · see citing works
RELIABILITY OF THE DETECTION OF THE BARYON ACOUSTIC PEAK
Martı́nez, V. J., Arnalte-Mur, P., Saar, E., de la Cruz, P., Pons-Bordería, M. J., Paredes, S., Fernández-Soto, A., & Tempel, E. (2009) · The Astrophysical Journal · doi:10.1088/0004-637x/696/1/l93 · Cited by 61 · see citing works
Wide Angle Redshift Distortions Revisited
Szapudi, I. (2004) · CERN Document Server (European Organization for Nuclear Research) · Cited by 57 · see citing works
Systematic effects in the sound horizon scale measurements
Guzik, J., Bernstein, G. M., & Smith, R. C. (2007) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2006.11385.x · Cited by 51 · see citing works
Labini, F. S., Vasilyev, N. L., Baryshev, Y. V., & López-Corredoira, M. (2009) · Astronomy and Astrophysics · doi:10.1051/0004-6361/200911987 · Cited by 49 · cited 1× · see citing works
“Other studies of the same data found similar results using the correlation function ξ(s) (Martinez 2009; Gaztanaga, Cabre & Hui 2009; Labini et al. 2009; Sanchez et al. 2009; Kazin et al. 2010), the power spectrum P (k) (Cole et al. 2005; Tegmark et al. 2006; Huetsi 2006; Reid et al. 2010), the…”
ResultMeasuring Angular Diameter Distances through Halo Clustering
Cooray, A. R., Hu, W., Dragan Huterer, A., & Joffre, M. (2001) · CERN Document Server (European Organization for Nuclear Research) · Cited by 47 · see citing works
Possible Detection of Baryonic Fluctuations in the Large‐Scale Structure Power Spectrum
Miller, C. J., Nichol, R. C., & Batuski, D. J. (2001) · The Astrophysical Journal · doi:10.1086/321468 · Cited by 46 · see citing works
Power spectrum of the SDSS luminous red galaxies: constraints on cosmological parameters
Hütsi, G. (2006) · Astronomy and Astrophysics · doi:10.1051/0004-6361:20065377 · Cited by 45 · see citing works
Large-scale structure in the H I Parkes All-Sky Survey: filling the voids with H I galaxies?
Basilakos, S., Plionis, M., Kovač, K., & Voglis, N. (2007) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2007.11781.x · Cited by 44 · cited 1× · see citing works
“For WALLABY we used a bias of 0.7 (based on the results found in the HIPASS survey; Basilakos et al. 2007).”
MethodInfluentialKazin, E. A., Blanton, M. R., Scoccimarro, R., McBride, C. K., & Berlind, A. A. (2010) · The Astrophysical Journal · doi:10.1088/0004-637x/719/2/1032 · Cited by 42 · cited 3× · see citing works
“Another motivation for our study is that the SDSS data after data release 3 (DR3) show more correlation on large scales than expected by ΛCDM and have no sign of a crossover to negative ξ up to 200h−1 Mpc (the ΛCDM prediction is 140h−1 Mpc) (Kazin et al. 2010).”
BackgroundMethodResultLabini, F. S., Vasilyev, N. L., Baryshev, Y. V., & López-Corredoira, M. (2009) · Springer Link (Chiba Institute of Technology) · doi:10.1051/0004-6361/200911987/pdf · Cited by 41 · see citing works
Dynamics of cosmological perturbations in position space
Bashinsky, S., & Bertschinger, E. (2002) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.65.123008 · Cited by 39 · cited 1× · see citing works
“Through this process each over-density of the original density perturbation field has evolved to become a centrally peaked perturbation surrounded by a spherical shell (Bashinsky & Bertschinger 2001, 2002; Eisenstein, Seo & White 2007).”
BackgroundDetermination of the Baryon Density from Large‐Scale Galaxy Redshift Surveys
Goldberg, D. M., & Strauss, M. A. (1998) · The Astrophysical Journal · doi:10.1086/305284 · Cited by 39 · cited 1× · see citing works
“Since the signal appears at very large scales, it is necessary to probe a large volume of the universe to decrease sample variance, which dominates the error on these scales (Tegmark 1997; Goldberg & Strauss 1998; Eisenstein, Hu & Tegmark 1998).”
BackgroundBashinsky, S., & Bertschinger, E. (2001) · Physical Review Letters · doi:10.1103/physrevlett.87.081301 · Cited by 37 · cited 1× · see citing works
“Through this process each over-density of the original density perturbation field has evolved to become a centrally peaked perturbation surrounded by a spherical shell (Bashinsky & Bertschinger 2001, 2002; Eisenstein, Seo & White 2007).”
BackgroundBaryon Acoustic OscillationsPreprint
Bassett, B. A., & Hložek, R. (2009) · arXiv (Cornell University) · doi:10.48550/arxiv.0910.5224 · Cited by 19 · see citing works
Galaxies as tracers of the mass distribution
Efstathiou, G. (2008) · Springer eBooks · doi:10.1007/bfb0118824 · Cited by 10 · cited 1× · see citing works
“Other authors have used the so called J3-weighting which optimises the error over all scales by weighting each scale differently (e.g. Efstathiou 1988; Loveday et al. 1995).”
MethodAorta Fluorescence Imaging by Using Confocal Microscopy
Wang, C., Tsai, J.-C., Chuang, C., Hsieh, Y., & Sun, C. (2011) · ISRN Cardiology · doi:10.5402/2011/215627 · Cited by 2 · see citing works
Flagged first, then by citations
Research works printed but not linked: 14
- Arnalte-Mur P. et al., 2011, MNRAS, submitted, preprint (arXiv:1101.1911) · arXiv
- Blake C. et al., 2011, preprint (arXiv:1105.2862) · arXiv
- Chuang C. H., Wang Y., 2011, preprint (arXiv:1102.2251) · arXiv
- Efstathiou G., 1988, in Lawrence A., ed., Proc. 3rd IRAS Conf., Comets to Cosmology. Springer, New York, p. 312
- Frigo M., Johnson S. G., 2005, Proc. IEEE 93, 216231
- Huetsi G., 2009, preprint (arXiv:0910.0492) · arXiv
- Jones D. H., Peterson B. A., Colless M., Saunders W., 2006, MNRAS, 369, 25
- Jones D. H. et al., 2009, preprint (arXiv:0903.5451) · arXiv
- Kitaura F. S., Jasche J., Metcalf R. B., 2009, preprint (arXiv:0911.1407) · arXiv
- Norberg P., Baugh C. M., Gaztanaga E., Croton D. J., preprint (arXiv:0810.1885) · arXiv
- Papai P., Szapudi I., 2008, preprint (arXiv:0802.2940) · arXiv
- Raccanelli A., Samushia L., Percival W. J., 2010, preprint (arXiv:1006. 1652)
- Sanchez A. G., Crocce M., Cabre A., Baugh C. M., Gaztanaga E., 2009, preprint (arXiv:0901.2570) · arXiv
- Szalay A. S., Matsubara T., Landy S. D., preprint (arXiv:astro-ph/9712007) · arXiv
Cited by
Sorted by citations
<i>Planck</i> 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 · see citing works
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 · see citing works
“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 6,875 · see citing works
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 · see citing works
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 · see citing works
“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 · see citing works
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 · see citing works
“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 · see citing works
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 · see citing works
“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 · see citing works
“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 <sup>*</sup>
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 · see citing works
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) · Repository@Nottingham (University of Nottingham) · doi:10.17863/cam.52 · Cited by 1,925 · see citing works
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 · see citing works
“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 · see citing works
“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 · see citing works
“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 2,002 · see citing works
f(T) teleparallel gravity and cosmology
Cai, Y.-F., Capozziello, S., Laurentis, M. D., & Saridakis, E. (2015) · Reports on progress in physics. Physical Society · doi:10.1088/0034-4885/79/10/106901 · Cited by 1,446 · see citing works
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 1,393 · see citing works
“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.”
MethodInfluentialAde, 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) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201525898 · Cited by 1,402 · see citing works
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 · see citing works
“…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 · see citing works
Wong, K. C., Suyu, S. H., Chen, G. C.-F., Rusu, C. E., Millon, M., Sluse, D., Bonvin, V., Fassnacht, C. D., Taubenberger, S., Auger, M. W., et al. (2019) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stz3094 · Cited by 1,178 · see citing works
“…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 · see citing works
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 · see citing works
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 1,082 · see citing works
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 · see citing works
“[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 · see citing works
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 · see citing works
“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 · see citing works
“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 954 · see citing works
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 · see citing works
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 · see citing works
“…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 · see citing works
“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 · see citing works
“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 · see citing works
“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 · see citing works
Self-citationMontePython 3: Boosted MCMC sampler and other features
Brinckmann, T., & Julien Lesgourgues, A. (2019) · Physics of the Dark Universe · doi:10.1016/j.dark.2018.100260 · Cited by 697 · see citing works
“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 · see citing works
“…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 · see citing works
Hubble constant hunter’s guide
Knox, L., & Millea, M. (2020) · Physical Review D · doi:10.1103/physrevd.101.043533 · Cited by 638 · see citing works
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 · see citing works
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 · see citing works
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., Aihara, H., et al. (2018) · Nippon Tenmon Gakkai obun kenkyu hokoku · doi:10.1093/pasj/psz010 · Cited by 444 · see citing works
“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 · see citing works
“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 · see citing works
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 · see citing works
Baumann, D., & McAllister, L. (2015) · Cambridge University Press eBooks · doi:10.1017/cbo9781316105733 · Cited by 535 · see citing works
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 · see citing works
“[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 · see citing works
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 · see citing works
“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 · see citing works
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 506 · see citing works
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 · see citing works
Self-citationPlanck 2015 results - XXIV. Cosmology from Sunyaev-Zeldovich cluster counts
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. (2015) · LA Referencia (Red Federada de Repositorios Institucionales de Publicaciones Científicas) · doi:10.1051/0004-6361/201525833 · Cited by 473 · see citing works
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 · see citing works
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 · see citing works
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 · see citing works
“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 · see citing works
“…(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 · see citing works
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 · see citing works
“± 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 · see citing works
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 · see citing works
“…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 · see citing works
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 · see citing works
“…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 · see citing works
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 404 · see citing works
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 · see citing works
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 · see citing works
“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…”
MethodCapozziello, S., D'Agostino, R., & Luongo, O. (2019) · International Journal of Modern Physics D · doi:10.1142/s0218271819300167 · Cited by 246 · see citing works
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 · see citing works
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 · see citing works
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 · see citing works
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 · see citing works
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 · see citing works
“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 · see citing works
“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 · see citing works
“[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 · see citing works
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 · see citing works
“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 · see citing works
“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 · see citing works
“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 337 · see citing works
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 · see citing works
“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 · see citing works
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 · see citing works
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 · see citing works
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 · see citing works
“(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 · see citing works
Yu, H.-B., Ratra, B., & Wang, F.-Y. (2017) · The Astrophysical Journal · doi:10.3847/1538-4357/aab0a2 · Cited by 298 · see citing works
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 366 · see citing works
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 322 · see citing works
“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 316 · see citing works
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 · see citing works
“…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 · see citing works
“…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 · see citing works
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 304 · see citing works
“…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 · see citing works
“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 · see citing works
“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 · see citing works
Flavor structures of charged fermions and massive neutrinos
Xing, Z. (2020) · Physics Reports · doi:10.1016/j.physrep.2020.02.001 · Cited by 301 · see citing works
“The final full-mission Planck measurements of the CMB anisotropies [87], combined with the BAO measurements [335, 336, 337], strongly support the”
Method
- 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
