Kinematic scaling relations of disc galaxies from ionised gas at z ∼ 1 and their connection with dark matter haloes

Open Access

Fig. 3.

Posterior distributions of the best-fitting TFR and FR. The distributions of low- and high-z disc galaxies are shown in blue (from Marasco et al. 2025) and pink (this work), respectively. The contours encompass the 0.393, 0.865, and 0.989 percentiles, corresponding to 1, 2, and 3σ in 2D distributions.

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