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arxiv: 1807.06209 · v4 · submitted 2018-07-17 · 🌌 astro-ph.CO

Recognition: 2 theorem links

· Lean Theorem

Planck 2018 results. VI. Cosmological parameters

A. A. Fraisse, A. Challinor, A. Ducout, A. Frolov, A. Gruppuso, A. H. Jaffe, A. J. Banday, A. Karakci, A. Lasenby, A. Lewis, A. Mangilli, A. Marcos-Caballero, A. Melchiorri, A. Mennella, A. Moss, A. Renzi, A.-S. Suur-Uski, A. Zacchei, A. Zonca, B. D. Wandelt, B. Partridge, B. P. Crill, B. Ruiz-Granados, B. Van Tent, C. Baccigalupi, C. Burigana, C. Combet, C. R. Lawrence, C. Rosset, C. Sirignano, D. Contreras, D. Herranz, D. Maino, D. Molinari, D. Paoletti, D. Scott, D. Tavagnacco, E. Calabrese, E. Di Valentino, E. Franceschi, E. Hivon, E. Keih\"anen, E. Mart\'inez-Gonz\'alez, E. P. S. Shellard, F. Boulanger, F. Cuttaia, F. Elsner, F. Finelli, F. Forastieri, F. K. Hansen, F. Levrier, F. Perrotta, F. Piacentini, F. R. Bouchet, F. Villa, G. de Zotti, G. Efstathiou, G. Lagache, G. Maggio, G. Morgante, G. Patanchon, G. Polenta, G. Rocha, G. Roudier, G. Sirri, H. C. Chiang, H. K. Eriksen, H. Kurki-Suonio, H. U. N{\o}rgaard-Nielsen, H. V. Peiris, I. K. Wehus, J. A. Rubi\~no-Mart\'in, J. A. Tauber, J. Aumont, J. Borrill, J. Carron, J. Chluba, J. Delabrouille, J. D. McEwen, J. E. Gudmundsson, J.-F. Cardoso, J. Fergusson, J. F. Mac\'ias-P\'erez, J. Gonz\'alez-Nuevo, J. Hamann, J. J. Bock, J. Kim, J. Lesgourgues, J.-L. Puget, J.-M. Delouis, J. M. Diego, J.-M. Lamarre, J.-P. Bernard, J. P. Rachen, J. R. Bond, J. Valiviita, K. Benabed, K. Ganga, K. Kiiveri, K. M. G\'orski, L. D. Spencer, L. Knox, L. Montier, L. Pagano, L. P. L. Colombo, L. Polastri, L. Salvati, L. Toffolatti, L. Valenziano, L. Vibert, M.-A. Miville-Desch\^enes, M. Ashdown, M. Ballardini, M. Bersanelli, M. Bucher, M. Douspis, M. Farhang, M. Frailis, M. Gerbino, M. Kunz, M. Lattanzi, M. Le Jeune, M. Liguori, M. Lilley, M. L\'opez-Caniego, M. Maris, M. Martinelli, M. Migliaccio, M. Millea, M. Reinecke, M. Remazeilles, M. Sandri, M. Savelainen, M. Tenti, M. Tomasi, M. White, N. Bartolo, N. Krachmalnicoff, N. Mandolesi, N. Mauri, N. Vittorio, O. Dor\'e, P. Bielewicz, P. B. Lilje, P. De Bernardis, P. G. Martin, Planck Collaboration: N. Aghanim, P. Lemos, P. M. Lubin, P. Natoli, P. R. Meinhold, P. Vielva, R. Battye, R. B. Barreiro, R. C. Butler, R. Fernandez-Cobos, R. Keskitalo, R. Sunyaev, R. T. G\'enova-Santos, S. Basak, S. D. M. White, S. Dusini, S. Galeotta, S. Galli, S. Gratton, S. Matarrese, S. Mitra, S. R. Hildebrandt, T. A. En{\ss}lin, T. Ghosh, T. S. Kisner, T. Trombetti, V. Lindholm, V. Pettorino, W. C. Jones, W. Handley, X. Dupac, Y. Akrami, Y. Fantaye, Y.-Z. Ma, Z. Huang

Pith reviewed 2026-05-10 14:36 UTC · model grok-4.3

classification 🌌 astro-ph.CO
keywords cosmological parametersCMB anisotropiesLambda CDM modeldark matter densitybaryon densityHubble constantneutrino massPlanck mission
0
0 comments X

The pith

Planck's final CMB measurements fix the standard flat six-parameter Lambda CDM parameters to high precision and find no compelling evidence for extensions.

A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.

The paper reports cosmological parameters from the complete set of Planck satellite observations of cosmic microwave background anisotropies. The data show strong consistency with the spatially flat six-parameter Lambda cold dark matter model when analyzed separately in temperature, polarization, and lensing channels and in combination. Derived values include a dark matter density of 0.120 plus or minus 0.001, baryon density of 0.0224 plus or minus 0.0001, scalar spectral index of 0.965 plus or minus 0.004, and optical depth of 0.054 plus or minus 0.007, with the angular acoustic scale determined to 0.03 percent precision. Inferred late-universe quantities such as the Hubble constant equal 67.4 plus or minus 0.5 kilometers per second per megaparsec under the base model. Combining with baryon acoustic oscillation data further constrains extra relativistic degrees of freedom to 2.99 plus or minus 0.17 and the sum of neutrino masses below 0.12 electronvolts while leaving the base model intact.

Core claim

A combined analysis gives dark matter density Omega_c h squared equal to 0.120 plus or minus 0.001, baryon density Omega_b h squared equal to 0.0224 plus or minus 0.0001, scalar spectral index n_s equal to 0.965 plus or minus 0.004, and optical depth tau equal to 0.054 plus or minus 0.007. We find good consistency with the standard spatially-flat six-parameter Lambda CDM cosmology having a power-law spectrum of adiabatic scalar perturbations from polarization, temperature, and lensing, separately and in combination. These results are only weakly dependent on the cosmological model and remain stable with somewhat increased errors in many commonly considered extensions. We find no compelling证据

What carries the argument

The likelihood fit of the observed CMB temperature, polarization, and lensing power spectra to the six-parameter base Lambda CDM model while marginalizing over standard foreground contributions.

If this is right

  • The Hubble constant is inferred to be 67.4 plus or minus 0.5 km/s/Mpc, the matter density parameter 0.315 plus or minus 0.007, and the fluctuation amplitude sigma_8 0.811 plus or minus 0.006 under the base model.
  • Extra relativistic degrees of freedom are limited to N_eff equal to 2.99 plus or minus 0.17 when the CMB results are combined with baryon acoustic oscillation data.
  • The sum of neutrino masses is constrained below 0.12 eV at 95 percent .
  • A mild preference for higher lensing amplitude appears in the spectra but is not supported by the lensing reconstruction or by baryon acoustic oscillation data in extended models.
  • The angular acoustic scale 100 theta_star is measured as 1.0411 plus or minus 0.0003.

Where Pith is reading between the lines

These are editorial extensions of the paper, not claims the author makes directly.

  • These parameter values supply a fixed benchmark that future large-scale structure surveys can use to test whether apparent tensions with local distance measurements persist.
  • The reported optical depth and spectral index place direct limits on the epoch of reionization and the simplest single-field inflation models.
  • If the mild lensing amplitude preference grows with improved data, it could motivate targeted searches for scale-dependent modifications to gravity or clustering.
  • The tight neutrino mass bound can be combined with terrestrial oscillation experiments to narrow the allowed mass hierarchy.

Load-bearing premise

The observed CMB power spectra are produced by the base spatially flat six-parameter Lambda CDM model plus standard foregrounds with no large unmodeled systematics or new physics that would change the shape of the likelihood surface.

What would settle it

An independent measurement from galaxy clustering or distance-ladder methods that yields a Hubble constant differing from 67.4 kilometers per second per megaparsec by many times the stated uncertainty while the CMB spectra themselves remain unchanged would falsify the consistency of the base model.

read the original abstract

We present cosmological parameter results from the final full-mission Planck measurements of the CMB anisotropies. We find good consistency with the standard spatially-flat 6-parameter $\Lambda$CDM cosmology having a power-law spectrum of adiabatic scalar perturbations (denoted "base $\Lambda$CDM" in this paper), from polarization, temperature, and lensing, separately and in combination. A combined analysis gives dark matter density $\Omega_c h^2 = 0.120\pm 0.001$, baryon density $\Omega_b h^2 = 0.0224\pm 0.0001$, scalar spectral index $n_s = 0.965\pm 0.004$, and optical depth $\tau = 0.054\pm 0.007$ (in this abstract we quote $68\,\%$ confidence regions on measured parameters and $95\,\%$ on upper limits). The angular acoustic scale is measured to $0.03\,\%$ precision, with $100\theta_*=1.0411\pm 0.0003$. These results are only weakly dependent on the cosmological model and remain stable, with somewhat increased errors, in many commonly considered extensions. Assuming the base-$\Lambda$CDM cosmology, the inferred late-Universe parameters are: Hubble constant $H_0 = (67.4\pm 0.5)$km/s/Mpc; matter density parameter $\Omega_m = 0.315\pm 0.007$; and matter fluctuation amplitude $\sigma_8 = 0.811\pm 0.006$. We find no compelling evidence for extensions to the base-$\Lambda$CDM model. Combining with BAO we constrain the effective extra relativistic degrees of freedom to be $N_{\rm eff} = 2.99\pm 0.17$, and the neutrino mass is tightly constrained to $\sum m_\nu< 0.12$eV. The CMB spectra continue to prefer higher lensing amplitudes than predicted in base -$\Lambda$CDM at over $2\,\sigma$, which pulls some parameters that affect the lensing amplitude away from the base-$\Lambda$CDM model; however, this is not supported by the lensing reconstruction or (in models that also change the background geometry) BAO data. (Abridged)

Editorial analysis

A structured set of objections, weighed in public.

Desk editor's note, referee report, simulated authors' rebuttal, and a circularity audit. Tearing a paper down is the easy half of reading it; the pith above is the substance, this is the friction.

Referee Report

0 major / 2 minor

Summary. The paper presents cosmological parameter results from the final full-mission Planck measurements of the CMB anisotropies. It finds good consistency with the standard spatially-flat 6-parameter ΛCDM cosmology from polarization, temperature, and lensing, separately and in combination. A combined analysis gives dark matter density Ω_c h² = 0.120±0.001, baryon density Ω_b h² = 0.0224±0.0001, scalar spectral index n_s = 0.965±0.004, and optical depth τ = 0.054±0.007. The angular acoustic scale is measured to 0.03% precision. The paper reports no compelling evidence for extensions to the base-ΛCDM model, with constraints on N_eff and neutrino mass when combined with BAO. It notes a >2σ preference for higher lensing amplitudes in the spectra but not supported by lensing reconstruction or BAO.

Significance. If the results hold, this is a landmark paper providing the definitive constraints on cosmological parameters from Planck CMB data. It demonstrates strong internal consistency and external cross-checks. The explicit acknowledgment of the lensing amplitude tension without claiming new physics is a positive aspect. The stability of the base model parameters under extensions and the tight bounds on additional parameters like neutrino mass add to its significance. This work sets the standard for ΛCDM parameters and has high impact in the field.

minor comments (2)
  1. [Abstract] Abstract: The quoted 0.03% precision on the angular acoustic scale (100θ_* = 1.0411 ± 0.0003) is a key result; the main text should explicitly reference the table or section deriving this quantity to aid readers.
  2. [Lensing discussion] Lensing amplitude discussion: The >2σ preference for higher lensing amplitudes is noted but would benefit from a direct cross-reference to the specific figure or table showing the deviation and its impact on parameters.

Simulated Author's Rebuttal

0 responses · 0 unresolved

We thank the referee for their positive assessment of the manuscript and for recommending acceptance. The referee's summary correctly reflects the main results, including the consistency with base-ΛCDM, the quoted parameter values, and the discussion of the lensing amplitude preference.

Circularity Check

0 steps flagged

No significant circularity detected

full rationale

The paper's derivation consists of standard likelihood maximization of the base flat ΛCDM model against the Planck temperature, polarization, and lensing spectra, yielding the quoted parameter values as direct fit outputs. Independent lensing reconstruction and external BAO constraints are invoked as cross-checks that do not reduce to the same fitted quantities by construction. No self-definitional loops, fitted inputs renamed as predictions, or load-bearing self-citations that collapse the central claim are present; the analysis remains externally falsifiable against the observed data and separate probes.

Axiom & Free-Parameter Ledger

1 free parameters · 2 axioms · 0 invented entities

The central claim rests on the assumption that the CMB data are generated by the standard flat ΛCDM model with adiabatic scalar perturbations; the six parameters are fitted quantities whose values constitute the result rather than independent inputs.

free parameters (1)
  • Ω_c h², Ω_b h², n_s, τ, H_0, A_s (or equivalent)
    The six base-ΛCDM parameters are determined by fitting the theoretical power spectra to the measured CMB data.
axioms (2)
  • domain assumption The universe is spatially flat and described by the 6-parameter ΛCDM model with a power-law spectrum of adiabatic scalar perturbations.
    Invoked throughout the base-model analysis and extension tests.
  • domain assumption Foreground contamination and instrumental systematics are adequately modeled by the chosen templates and masks.
    Required for the likelihood to be interpreted as cosmological.

pith-pipeline@v0.9.0 · 6809 in / 1566 out tokens · 43356 ms · 2026-05-10T14:36:29.337717+00:00 · methodology

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Reference graph

Works this paper leans on

299 extracted references · 285 canonical work pages · cited by 165 Pith papers · 4 internal anchors

  1. [1]

    N., Canac, N., Horiuchi, S., & Kaplinghat, M., Astrophysical and Dark Matter Interpretations of Extended Gamma-Ray Emission from the Galactic Center

    Abazajian, K. N., Canac, N., Horiuchi, S., & Kaplinghat, M., Astrophysical and Dark Matter Interpretations of Extended Gamma-Ray Emission from the Galactic Center . 2014, , 90, 023526, 1402.4090

    work page arXiv 2014

  2. [2]

    Abbott, B. et al. , GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral . 2017, Phys. Rev. Lett., 119, 161101, 1710.05832

    work page internal anchor Pith review arXiv 2017

  3. [3]

    A gravitational-wave standard siren measurement of the Hubble constant

    Abbott , B. P., Abbott , R., Abbott , T. D., et al. , A gravitational-wave standard siren measurement of the Hubble constant . 2017, , 551, 85, 1710.05835

    work page Pith review arXiv 2017

  4. [4]

    Abe, K. et al. , Atmospheric neutrino oscillation analysis with external constraints in Super-Kamiokande I-IV . 2018, Phys. Rev., D97, 072001, 1710.09126

    work page arXiv 2018

  5. [5]

    Adamson, P. et al. , Constraints on Oscillation Parameters from _e Appearance and _ Disappearance in NOvA . 2017, , 118, 231801, 1703.03328

    work page Pith review arXiv 2017

  6. [6]

    E., Huang, Y., Watts, D

    Addison, G. E., Huang, Y., Watts, D. J., et al. , Quantifying discordance in the 2015 Planck CMB spectrum . 2016, , 818, 132, 1511.00055

    work page arXiv 2015

  7. [7]

    E., Watts , D

    Addison , G. E., Watts , D. J., Bennett , C. L., et al. , Elucidating CDM: Impact of Baryon Acoustic Oscillation Measurements on the Hubble Constant Discrepancy . 2018, , 853, 119, 1707.06547

    work page arXiv 2018

  8. [8]

    Ade, P. A. R. et al. , BICEP2 / Keck Array x: Constraints on Primordial Gravitational Waves using Planck, WMAP, and New BICEP2/Keck Observations through the 2015 Season . 2018, , 121, 221301, 1810.05216

    work page Pith review arXiv 2015

  9. [9]

    Adelberger, E. G. et al. , Solar fusion cross sections II: the pp chain and CNO cycles . 2011, Rev. Mod. Phys., 83, 195, 1004.2318

    work page arXiv 2011

  10. [10]

    Agafonova, N. et al. , Final results of the search for _ _ e oscillations with the OPERA detector in the CNGS beam . 2018, JHEP, 06, 151, 1803.11400

    work page arXiv 2018

  11. [11]

    2019, arXiv e-prints, arXiv:1904.01016

    Agrawal, P., Cyr-Racine, F.-Y., Pinner, D., & Randall, L., Rock 'n' Roll Solutions to the Hubble Tension . 2019, arXiv e-prints, 1904.01016

    work page arXiv 2019

  12. [12]

    Aguilar-Arevalo, A. et al. , Evidence for neutrino oscillations from the observation of anti-neutrino(electron) appearance in a anti-neutrino(muon) beam . 2001, Phys. Rev., D64, 112007, hep-ex/0104049

    work page arXiv 2001

  13. [13]

    Aguilar-Arevalo, A. A. et al. , Significant Excess of ElectronLike Events in the MiniBooNE Short-Baseline Neutrino Experiment . 2018, , 121, 221801, 1805.12028

    work page arXiv 2018

  14. [14]

    Akrami, R

    Akrami , Y., Kallosh , R., Linde , A., & Vardanyan , V., Dark energy, -attractors, and large-scale structure surveys . 2018, , 6, 041, 1712.09693

    work page arXiv 2018

  15. [15]

    Alam, S. et al. , The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample . 2017, , 470, 2617, 1607.03155

    work page Pith review arXiv 2017

  16. [16]

    & Paczynski , B., An evolution free test for non-zero cosmological constant

    Alcock , C. & Paczynski , B., An evolution free test for non-zero cosmological constant . 1979, , 281, 358

    1979

  17. [17]

    & Hirata , C

    Ali-Ha \"i moud , Y. & Hirata , C. M., Ultrafast effective multilevel atom method for primordial hydrogen recombination . 2010, , 82, 063521, 1006.1355

    work page arXiv 2010

  18. [18]

    & Hirata, C

    Ali-Haimoud, Y. & Hirata, C. M., HyRec: A fast and highly accurate primordial hydrogen and helium recombination code . 2011, , 83, 043513, 1011.3758

    work page arXiv 2011

  19. [19]

    Allison, P

    Allison, R., Caucal, P., Calabrese, E., Dunkley, J., & Louis, T., Towards a cosmological neutrino mass detection . 2015, Phys. Rev., D92, 123535, 1509.07471

    work page arXiv 2015

  20. [20]

    Almazán, H. et al. , Sterile neutrino exclusion from the STEREO experiment with 66 days of reactor-on data . 2018, ArXiv e-prints, 1806.02096

    work page arXiv 2018

  21. [21]

    Coupled Quintessence

    Amendola, L., Coupled quintessence . 2000, Phys. Rev., D62, 043511, astro-ph/9908023

    work page Pith review arXiv 2000

  22. [22]

    Amendola, M

    Amendola, L., Kunz, M., & Sapone, D., Measuring the dark side (with weak lensing) . 2008, , 0804, 013, 0704.2421

    work page arXiv 2008

  23. [23]

    Anderson, L. et al. , The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Baryon Acoustic Oscillations in the Data Release 10 and 11 galaxy samples . 2014, , 441, 24, 1312.4877

    work page arXiv 2014

  24. [24]

    Archidiacono, S

    Archidiacono, M., Gariazzo, S., Giunti, C., et al. , Pseudoscalar—sterile neutrino interactions: reconciling the cosmos with neutrino oscillations . 2016, JCAP, 1608, 067, 1606.07673

    work page arXiv 2016

  25. [25]

    Archidiacono, D

    Archidiacono, M., Hooper, D. C., Murgia, R., et al. , Constraining Dark Matter-Dark Radiation interactions with CMB, BAO, and Lyman- . 2019, JCAP, 1910, 055, 1907.01496

    work page arXiv 2019

  26. [26]

    The universal galaxy cluster pressure profile from a representative sample of nearby systems (REXCESS) and the Y_SZ-M_500 relation

    Arnaud , M., Pratt , G. W., Piffaretti , R., et al. , The universal galaxy cluster pressure profile from a representative sample of nearby systems (REXCESS) and the Y _ SZ - M _ 500 relation . 2010, , 517, A92, 0910.1234

    work page Pith review arXiv 2010

  27. [27]

    Ashenfelter, J. et al. , First search for short-baseline neutrino oscillations at HFIR with PROSPECT . 2018, , 121, 251802, 1806.02784

    work page arXiv 2018

  28. [28]

    Ata, M. et al. , The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: first measurement of baryon acoustic oscillations between redshift 0.8 and 2.2 . 2018, , 473, 4773, 1705.06373

    work page arXiv 2018

  29. [29]

    Aubourg, \'E . et al. , Cosmological implications of baryon acoustic oscillation measurements . 2015, , 92, 123516, 1411.1074

    work page arXiv 2015

  30. [30]

    Conservative Constraints on Early Cosmology: an illustration of the Monte Python cosmological parameter inference code

    Audren, B., Lesgourgues, J., Benabed, K., & Prunet, S., Conservative Constraints on Early Cosmology: an illustration of the Monte Python cosmological parameter inference code . 2013, JCAP, 1302, 001, 1210.7183

    work page Pith review arXiv 2013

  31. [31]

    Aver, K.A

    Aver, E., Olive, K. A., & Skillman, E. D., The effects of He I ?10830 on helium abundance determinations . 2015, , 1507, 011, 1503.08146

    work page arXiv 2015

  32. [32]

    , A Comparison of Cosmological Parameters Determined from CMB Temperature Power Spectra from the South Pole Telescope and the Planck Satellite

    Aylor , K., Hou , Z., Knox , L., et al. , A Comparison of Cosmological Parameters Determined from CMB Temperature Power Spectra from the South Pole Telescope and the Planck Satellite . 2017, , 850, 101, 1706.10286

    work page arXiv 2017

  33. [33]

    Strong constraints on cosmological gravity from GW170817 and GRB 170817A

    Baker, T., Bellini, E., Ferreira, P. G., et al. , Strong constraints on cosmological gravity from GW170817 and GRB 170817A . 2017, Phys. Rev. Lett., 119, 251301, 1710.06394

    work page Pith review arXiv 2017

  34. [34]

    Banados, E. et al. , An 800 million solar mass black hole in a significantly neutral universe at redshift 7.5 . 2018, Nature, 553, 473, 1712.01860

    work page arXiv 2018

  35. [35]

    Weak Gravitational Lensing

    Bartelmann, M. & Schneider, P., Weak Gravitational Lensing. 2001, Phys. Rept., 340, 291, astro-ph/9912508

    work page Pith review arXiv 2001

  36. [36]

    Baumann , D

    Baumann, D., Green, D., & Wallisch, B., Searching for light relics with large-scale structure . 2018, JCAP, 1808, 029, 1712.08067

    work page arXiv 2018

  37. [37]

    Bautista, J. E. et al. , Measurement of baryon acoustic oscillation correlations at z=2.3 with SDSS DR12 Ly -Forests . 2017, , 603, A12, 1702.00176

    work page arXiv 2017

  38. [38]

    Bautista, J. E. et al. , The SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Baryon Acoustic Oscillations at redshift of 0.72 with the DR14 Luminous Red Galaxy Sample . 2018, , 863, 110, 1712.08064

    work page arXiv 2018

  39. [39]

    Conceptual aspects and cosmological predictions

    Belgacem, E., Dirian, Y., Foffa, S., & Maggiore, M., Nonlocal gravity. Conceptual aspects and cosmological predictions . 2018, JCAP, 1803, 002, 1712.07066

    work page arXiv 2018

  40. [40]

    Maximal freedom at minimum cost: linear large-scale structure in general modifications of gravity

    Bellini , E. & Sawicki , I., Maximal freedom at minimum cost: linear large-scale structure in general modifications of gravity . 2014, , 7, 050, 1404.3713

    work page Pith review arXiv 2014

  41. [41]

    Ben Achour, M

    Ben Achour, J., Crisostomi, M., Koyama, K., et al. , Degenerate higher order scalar-tensor theories beyond Horndeski up to cubic order . 2016, JHEP, 12, 100, 1608.08135

    work page arXiv 2016

  42. [42]

    Bennett, C. et al. , Nine-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Final Maps and Results . 2013, , 208, 20, 1212.5225

    work page arXiv 2013

  43. [43]

    Bennett, C. L. et al. , First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Preliminary Maps and Basic Results. 2003, , 148, 1, astro-ph/0302207

    work page arXiv 2003

  44. [44]

    L., Verde, L., & Riess, A

    Bernal, J. L., Verde, L., & Riess, A. G., The trouble with H_0 . 2016, JCAP, 1610, 019, 1607.05617

    work page arXiv 2016

  45. [45]

    Improved cosmological constraints from a joint analysis of the SDSS-II and SNLS supernova samples

    Betoule , M., Kessler , R., Guy , J., et al. , Improved cosmological constraints from a joint analysis of the SDSS-II and SNLS supernova samples . 2014, , 568, A22, 1401.4064

    work page Pith review arXiv 2014

  46. [46]

    , Improved photometric calibration of the SNLS and the SDSS supernova surveys

    Betoule , M., Marriner , J., Regnault , N., et al. , Improved photometric calibration of the SNLS and the SDSS supernova surveys . 2013, , 552, A124, 1212.4864

    work page arXiv 2013

  47. [47]

    The 6dF Galaxy Survey: Baryon Acoustic Oscillations and the Local Hubble Constant

    Beutler, F., Blake, C., Colless, M., et al. , The 6dF Galaxy Survey: Baryon Acoustic Oscillations and the Local Hubble Constant . 2011, , 416, 3017, 1106.3366

    work page Pith review arXiv 2011

  48. [48]

    , The 6dF Galaxy Survey: z 0 measurement of the growth rate and _8

    Beutler, F., Blake, C., Colless, M., et al. , The 6dF Galaxy Survey: z 0 measurement of the growth rate and _8 . 2012, , 423, 3430, 1204.4725

    work page arXiv 2012

  49. [49]

    , The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: anisotropic galaxy clustering in Fourier space

    Beutler , F., Seo , H.-J., Saito , S., et al. , The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: anisotropic galaxy clustering in Fourier space . 2017, , 466, 2242, 1607.03150

    work page arXiv 2017

  50. [50]

    Beutler, F. et al. , The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: baryon acoustic oscillations in the Fourier space . 2017, , 464, 3409, 1607.03149

    work page arXiv 2017

  51. [51]

    A Joint Analysis of BICEP2/Keck Array and Planck Data

    BICEP2/Keck Array and Planck Collaborations , Joint Analysis of BICEP2/Keck Array and Planck Data . 2015, , 114, 101301, 1502.00612

    work page Pith review arXiv 2015

  52. [52]

    , On the Nature of Hydrostatic Equilibrium in Galaxy Clusters

    Biffi , V., Borgani , S., Murante , G., et al. , On the Nature of Hydrostatic Equilibrium in Galaxy Clusters . 2016, , 827, 112, 1606.02293

    work page arXiv 2016

  53. [53]

    Blake, C. et al. , The WiggleZ Dark Energy Survey: Joint measurements of the expansion and growth history at z < 1 . 2012, , 425, 405, 1204.3674

    work page arXiv 2012

  54. [54]

    Blake, C. et al. , Galaxy And Mass Assembly (GAMA): improved cosmic growth measurements using multiple tracers of large-scale structure . 2013, , 436, 3089, 1309.5556

    work page arXiv 2013

  55. [55]

    & Schneider , J., Gravitational lensing effect on the fluctuations of the cosmic background radiation

    Blanchard , A. & Schneider , J., Gravitational lensing effect on the fluctuations of the cosmic background radiation . 1987, , 184, 1

    1987

  56. [56]

    The Cosmic Linear Anisotropy Solving System (CLASS) II: Approximation schemes

    Blas, D., Lesgourgues, J., & Tram, T., The Cosmic Linear Anisotropy Solving System (CLASS) II: Approximation schemes . 2011, , 1107, 034, 1104.2933

    work page internal anchor Pith review arXiv 2011

  57. [57]

    Blomqvist, M. et al. , Baryon acoustic oscillations from the cross-correlation of Ly absorption and quasars in eBOSS DR14 . 2019, Astron. Astrophys., 629, A86, 1904.03430

    work page arXiv 2019

  58. [58]

    A., The extended ROSAT-ESO Flux Limited X-ray Galaxy Cluster Survey (REFLEX II) IV

    B \"o hringer, H., Chon, G., & Collins, C. A., The extended ROSAT-ESO Flux Limited X-ray Galaxy Cluster Survey (REFLEX II) IV. X-ray Luminosity Function and First Constraints on Cosmological Parameters . 2014, , 570, A31, 1403.2927

    work page arXiv 2014

  59. [59]

    , The extended Northern ROSAT Galaxy Cluster Survey (NORAS II) I

    B \"o hringer, H., Chon, G., Retzlaff, J., et al. , The extended Northern ROSAT Galaxy Cluster Survey (NORAS II) I. Survey Construction and First Results . 2017, , 153, 220, 1704.06489

    work page arXiv 2017

  60. [60]

    Borsanyi, S. et al. , Calculation of the axion mass based on high-temperature lattice quantum chromodynamics . 2016, Nature, 539, 69, 1606.07494

    work page arXiv 2016

  61. [61]

    Reionization after Planck: The Derived Growth of the Cosmic Ionizing Emissivity now matches the Growth of the Galaxy UV Luminosity Density

    Bouwens, R. J., Illingworth, G. D., Oesch, P. A., et al. , Reionization after Planck : The Derived Growth of the Cosmic Ionizing Emissivity Now Matches the Growth of the Galaxy UV Luminosity Density . 2015, , 811, 140, 1503.08228

    work page Pith review arXiv 2015

  62. [62]

    D., Rogers, A

    Bowman, J. D., Rogers, A. E. E., Monsalve, R. A., Mozdzen, T. J., & Mahesh, N., An Absorption Profile Centred at 78 Megahertz in the Sky-Averaged Spectrum. 2018, Nature, 555, 67

    2018

  63. [63]

    , A combined view of sterile-neutrino constraints from CMB and neutrino oscillation measurements

    Bridle , S., Elvin-Poole , J., Evans , J., et al. , A combined view of sterile-neutrino constraints from CMB and neutrino oscillation measurements . 2017, Physics Letters B, 764, 322, 1607.00032

    work page arXiv 2017

  64. [64]

    MontePython 3: boosted MCMC sampler and other features

    Brinckmann, T. & Lesgourgues, J., MontePython 3: boosted MCMC sampler and other features . 2019, Phys. Dark Univ., 24, 100260, 1804.07261

    work page Pith review arXiv 2019

  65. [65]

    Interacting Dark Sec- tor and Precision Cosmology,

    Buen-Abad, M. A., Schmaltz, M., Lesgourgues, J., & Brinckmann, T., Interacting Dark Sector and Precision Cosmology . 2018, JCAP, 1801, 008, 1708.09406

    work page arXiv 2018

  66. [66]

    Calabrese, A

    Calabrese, E., Slosar, A., Melchiorri, A., Smoot, G. F., & Zahn, O., Cosmic Microwave Weak lensing data as a test for the dark universe . 2008, , 77, 123531, 0803.2309

    work page arXiv 2008

  67. [67]

    2015, , 91, 063003, 1411.4647

    Calore, F., Cholis, I., McCabe, C., & Weniger, C., A Tale of Tails: Dark Matter Interpretations of the Fermi GeV Excess in Light of Background Model Systematics . 2015, , 91, 063003, 1411.4647

    work page arXiv 2015

  68. [68]

    Current unknowns in the three neutrino framework

    Capozzi, F., Lisi, E., Marrone, A., & Palazzo, A., Current unknowns in the three neutrino framework . 2018, Prog. Part. Nucl. Phys., 102, 48, 1804.09678

    work page Pith review arXiv 2018

  69. [69]

    2017, , 3, 056, 1611.06088

    Cardona , W., Kunz , M., & Pettorino , V., Determining H _ 0 with Bayesian hyper-parameters . 2017, , 3, 056, 1611.06088

    work page arXiv 2017

  70. [70]

    2017, , 1705, 035, 1701.01712

    Carron, J., Lewis, A., & Challinor, A., Internal delensing of Planck CMB temperature and polarization . 2017, , 1705, 035, 1701.01712

    work page arXiv 2017

  71. [71]

    Carter, F

    Carter, P., Beutler, F., Percival, W. J., et al. , Low Redshift Baryon Acoustic Oscillation Measurement from the Reconstructed 6-degree Field Galaxy Survey . 2018, , 481, 2371, 1803.01746

    work page arXiv 2018

  72. [72]

    2017, Phys

    Casas, S., Kunz, M., Martinelli, M., & Pettorino, V., Linear and non-linear Modified Gravity forecasts with future surveys . 2017, Phys. Dark Univ., 18, 73, 1703.01271

    work page arXiv 2017

  73. [73]

    Charles, E. et al. , Sensitivity Projections for Dark Matter Searches with the Fermi Large Area Telescope . 2016, Phys. Rept., 636, 1, 1605.02016

    work page arXiv 2016

  74. [74]

    A 2 per cent Hubble constant measurement from standard sirens within 5 years

    Chen, H.-Y., Fishbach, M., & Holz, D. E., A two per cent Hubble constant measurement from standard sirens within five years . 2018, Nature, 562, 545, 1712.06531

    work page Pith review arXiv 2018

  75. [75]

    Cheung, P

    Cheung , C., Fitzpatrick , A. L., Kaplan , J., Senatore , L., & Creminelli , P., The effective field theory of inflation . 2008, Journal of High Energy Physics, 3, 014, 0709.0293

    work page arXiv 2008

  76. [76]

    & Sunyaev , R

    Chluba , J. & Sunyaev , R. A., Induced two-photon decay of the 2s level and the rate of cosmological hydrogen recombination . 2006, , 446, 39, astro-ph/0508144

    work page arXiv 2006

  77. [77]

    & Thomas , R

    Chluba , J. & Thomas , R. M., Towards a complete treatment of the cosmological recombination problem . 2011, , 412, 748, 1010.3631

    work page arXiv 2011

  78. [78]

    2015, JCAP, 1510, 011, 1505.02795

    Chu, X., Dasgupta, B., & Kopp, J., Sterile neutrinos with secret interactions—lasting friendship with cosmology . 2015, JCAP, 1510, 011, 1505.02795

    work page arXiv 2015

  79. [79]

    2009, Nucl

    Cirelli, M., Kadastik, M., Raidal, M., & Strumia, A., Model-independent implications of the e+-, anti-proton cosmic ray spectra on properties of Dark Matter . 2009, Nucl. Phys., B813, 1, [Addendum: Nucl. Phys.B873,530(2013)], 0809.2409

    work page arXiv 2009

  80. [80]

    Cole , W

    Cole , S., Percival , W. J., Peacock , J. A., et al. , The 2dF Galaxy Redshift Survey: power-spectrum analysis of the final data set and cosmological implications . 2005, , 362, 505, arXiv:astro-ph/0501174

    work page arXiv 2005

Showing first 80 references.