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Table 3.

Cosmological parameters at the 68% c.l. when varying the EoS for dark energy.

Experiment Ωm σ8 w0 wa
Euclid-like, 1% SR, T08 0.3164 ± 0.0013 0.8121 ± 0.0012
Euclid-like, 5% SR, T08 0.3165 ± 0.0018 0.8122 ± 0.0033 −1.000 ± 0.010
Euclid-like, 5% SR, D16 0.3066 ± 0.0020 0.8153 ± 0.0034 −1.095 ± 0.012
Euclid-like, 10% SR, T08 0.3163 ± 0.0027 0.8121 ± 0.0051

LSST-like, 1% SR, T08 −1.003 ± 0.010
LSST-like, 5% SR, T08 0.3167 ± 0.0020 −1.000 ± 0.012
LSST-like, 10% SR, T08 0.3165 ± 0.0030 0.8118 ± 0.0050 −1.000 ± 0.014

WFIRST-like, 1% SR, T08 0.8342 ± 0.0036 −1.000 ± 0.015
WFIRST-like, 5% SR, T08 0.3169 ± 0.0038 0.8119 ± 0.0050 −0.998 ± 0.021
WFIRST-like, 10% SR, T08 0.3167 ± 0.0044 0.8122 ± 0.0079 −0.999 ± 0.024

Notes. We report the results for the Euclid-like, LSST-like, and WFIRST-like simulated experiments at different levels of scaling relation precision. We show the comparison between the T08 and D16 mass function formulations only for the Euclid-like experiment.

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