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Unveiling the trends between dust attenuation and galaxy properties at z ∼ 2-12 with the James Webb Space Telescope

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Moderate correlations exist between dust attenuation parameters and fundamental galaxy properties, helping to unveil trends.
Lower V-band attenuation is associated with steeper dust slopes and stronger UV bumps in high-redshift galaxies.
Young stars and bursty galaxies might preferentially destroy small dust grains, influencing the dust distribution.
Positive correlation between the UV bump parameter and oxygen abundance suggests links between dust properties and gas metallicity.

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Analysis unveils correlations between dust attenuation curves and galaxy properties, suggesting key physical mechanisms in galaxy formation.

Markov et al. (2025) studied this question.

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Analysis unveils correlations between dust attenuation curves and galaxy properties, suggesting key physical mechanisms in galaxy formation.