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Table 5.

Forecast constraints on wCDM cosmological parameters.

wCDM model, fsky = 70% case
σ(H0) σ(w) σbh2) σch2) σ(τ) σ(ns) σ(109As) σΛ)
CMB* + CIB 0.561 0.0308 0.000143 0.00118 0.0170 0.00434 0.0730 0.00480
+CIB×CMB lensing 2.98% 2.20% 0.577% 1.13% 27.7% 0.756% 30.7% 2.93%
+CIB×ISW 56.4% 80.1% 10.1% 50.8% 43.4% 22.0% 38.7% 29.4%

wCDM model, fsky = 40% case

σ(H0) σ(w) σbh2) σch2) σ(τ) σ(ns) σ(109As) σΛ)
CMB* + CIB 0.656 0.0330 0.000144 0.00121 0.0170 0.00437 0.0730 0.00575
+CIB×CMB lensing 2.91% 1.85% 0.322% 0.749% 20.2% 0.553% 22.3% 3.15%
+ CIB×ISW 55.4% 79.5% 9.15% 43.6% 36.5% 18.8% 33.2% 29.8%

Notes. The upper and lower tables show our results in the fsky = 70% and fsky = 40% cases, respectively. In each table, the first line shows the predicted 1σ errors from CMB* + CIB constraints. The second line shows the improvements on these errors (i.e. relative reduction in percent) after adding the CIB×CMB lensing constraints. The last line shows the further improvement thanks to CIB×ISW constraints, using the {CMB + CIB +CMB×CIB lensing} case as a reference. The constraints on ΩΛ are derived from the other parameters (and are not originally part of the Fisher analysis).

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