Table 7.
Marginalized values and 68% confidence regions for cosmological parameters obtained combining Planck TT,TE,EE+lowE with other data sets, assuming the (μ, η) parameterization of modified gravity.
With CMB lensing |
Without CMB lensing |
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Planck | Planck | Planck | Planck | Planck | Planck | |
Parameter | +SNe+BAO | +BAO/RSD+WL | +SNe+BAO | +BAO/RSD+WL | ||
μ0 − 1 …… |
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η0 − 1 …… |
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Σ0 − 1 …… | 0.100 ± 0.093 | 0.106 ± 0.086 |
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τ …… |
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0.0524 ± 0.0075 | 0.0504 ± 0.0080 | 0.0505 ± 0.0080 | 0.0526 ± 0.0079 |
H0 [ km s−1 Mpc−1] …… | 68.20 ± 0.63 | 68.19 ± 0.45 | 68.09 ± 0.45 | 68.23 ± 0.71 | 68.26 ± 0.48 | 68.09 ± 0.46 |
σ8 …… |
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S8 …… | 0.817 ± 0.037 |
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⟨d2⟩1/2 [arcmin] …… |
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2.529 ± 0.049 | 2.453 ± 0.032 |
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2.456 ± 0.043 |
Σ0S8 …… | 0.898 ± 0.067 |
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Δχ2 …… | −4.6 | −5.5 | −1.2 | −10.2 | −11.0 | −0.7 |
Notes. The Δχ2 values are computed with respect to the best-fit ΛCDM cosmology, using the same data combination. The quantity ⟨d2⟩1/2 is the root-mean-square CMB lensing deflection angle, which is pulled high by the CMB data unless galaxy lensing (WL) or CMB lensing are included. The combination Σ0S8 is approximately the lensing amplitude parameter best constrained by the DES WL data at lower redshift.
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