Intermediate-redshift galaxies show systematically higher dust attenuation at fixed star formation rate surface density than local galaxies, with the excess strongest for galaxies below the star-forming main sequence.
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Main-sequence galaxies at z~1.1–1.6 host extended CO, [C I], and dust disks with roughly constant gas fraction and depletion time out to 2 Re, supporting steady accretion rather than mergers.
citing papers explorer
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The MAGPI Survey: Evidence for Non-Universal Resolved Dust Attenuation Relations Beyond the Local Universe
Intermediate-redshift galaxies show systematically higher dust attenuation at fixed star formation rate surface density than local galaxies, with the excess strongest for galaxies below the star-forming main sequence.
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NOEMA3D: extended CO, [C I] and dust in massive star-forming main sequence galaxies at cosmic noon
Main-sequence galaxies at z~1.1–1.6 host extended CO, [C I], and dust disks with roughly constant gas fraction and depletion time out to 2 Re, supporting steady accretion rather than mergers.