Euclid preparation - L. Calibration of the halo linear bias in Λ(v)CDM cosmologies

Open Access

Fig. 6

Marginalized 68% and 95% confidence level contours on the model parameters presented in Eqs. (24) to (27). We calibrated our model using the subset of PICCOLO simulations C0–C10. (See Table 2 for the best fit and confidence levels.)

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