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Fig. 4.

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Contribution of the dusty galaxies in the GOODS-N overdensity to the cosmic SFRD, ψ, at z ∼ 5.2. The red star represents the SFRD derived from spectroscopically confirmed galaxies, while the blue star also includes the contribution from galaxies with photometric redshifts. The purple curves show the total SFRD as a function of redshift: the dashed line corresponds to the Madau & Dickinson (2014) result, obtained by correcting the UV SFRD for dust attenuation, and the solid line to Fujimoto et al. (2024), obtained by summing the obscured (IR) and unobscured (UV) contributions. At z ∼ 5, the dust-obscured SFRD estimates from Traina et al. (2024) and Sun et al. (2025) are shown as an orange diamond and circle, respectively. The orange and blue shaded areas represent the obscured and unobscured SFRD, respectively, from Zavala et al. (2021).

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