Fig. 9.

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ISW amplitude
, computed from power spectra ratios for 777 simulations spanning a wide range of wCDM cosmological parameters. The main scatter plot shows
as a function of Ωm, with points colour-coded by w. Three representative simulations (Sim 127, Sim 401, and Sim 742) are highlighted with unfilled black markers. The horizontal dashed line indicates the fiducial ΛCDM expectation
. The inset histogram shows the distribution of the
, also showing a broad variation in ISW strength across cosmological models.
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