Figure 6.
![Observed peculiar velocity statistic ψ1 as a function of the pair separation r. The ΛCDM model, fσ8 = 0.4, predicted for CF3 galaxies is shown as a black solid line. Scattered points with error bars represent results obtained from observed peculiar velocities of the CF3 galaxies, derived by considering different values of the Hubble constant H0 = [66, 68, 70, 72, 73, 74, 75, 76, 77, 79] km s−1 Mpc−1.](https://oup.silverchair-cdn.com/oup/backfile/Content_public/Journal/mnras/486/1/10.1093_mnras_stz901/1/stz901fig6.jpeg?Expires=1749760105&Signature=aYYxJOgx0frO5--q9jx7-cGHbsAUUVZ7629ASVtm2Fo8AwF0I7gZzuzBosBM~1x54tcjlseBVLLh2egUJWsRg5R5n3e-clv9KhhTOi5ICZZV1INfmFq6ag1GJ4JruEnIFuy6BZzM7djvHbMHlwfxjxB4Lv5VcfbLaYWJmHZ9lSeKqnPwN0MVboHIQvYYNs6jwTjxml~3onFY3tsyM~6UGnHFDtFhdiCea~royRMJMukAZyrFDA75Bwk0vbaWH2rB0Sateok34nfeXJ2WbLVMopNdRVgr~lkiNOgqAZtLMaSngv8XXBA3TWO5vtVeBIeS3XDsaPCTAr-xdez~wfGPKg__&Key-Pair-Id=APKAIE5G5CRDK6RD3PGA)
Observed peculiar velocity statistic ψ1 as a function of the pair separation r. The ΛCDM model, fσ8 = 0.4, predicted for CF3 galaxies is shown as a black solid line. Scattered points with error bars represent results obtained from observed peculiar velocities of the CF3 galaxies, derived by considering different values of the Hubble constant H0 = [66, 68, 70, 72, 73, 74, 75, 76, 77, 79] km s−1 Mpc−1.
