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Table 4.

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

Experiment BM, 0 α σlnM β
Euclid-like, 1% SR, T08 0.0 ± 0.001 0.0 ± 0.0020
Euclid-like, 5% SR, T08 0.0 ± 0.005 0.0 ± 0.010 0.2002 ± 0.0084
Euclid-like, 5% SR, D16 −0.0007 ± 0.0047 0.002 ± 0.010 0.1935 ± 0.0088 0.1250 ± 0.0034
Euclid-like, 10% SR, T08 0.0 ± 0.010 0.0 ± 0.020 0.201 ± 0.015 0.1245 ± 0.0051

LSST-like, 1% SR, T08 0.0 ± 0.0011 0.0 ± 0.0019 0.2001 ± 0.0018 0.1250 ± 0.0011
LSST-like, 5% SR, T08 0.0 ± 0.0047 0.001 ± 0.010 0.1995 ± 0.0087
LSST-like, 10% SR, T08 0.0 ± 0.010 0.0 ± 0.019 0.201 ± 0.015 0.1248 ± 0.0064

WFIRST-like, 1% SR, T08 0.0 ± 0.0010 0.1250 ± 0.0013
WFIRST-like, 5% SR, T08 0.0 ± 0.0049 0.0 ± 0.010 0.200 ± 0.010 0.1249 ± 0.0053
WFIRST-like, 10% SR, T08 0.0 ± 0.010 0.0 ± 0.019 0.200 ± 0.018 0.1249 ± 0.0077

Notes. We report 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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